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To celebrate the thrill of space exploration and the joy of learning, we've created a special crossword puzzle built entirely from this week's top Space.com stories. It's a fun, brain-tickling way to revisit the highlights, whether you're a casual stargazer or a die-hard astrophysics fan.
Expect clues that span planetary science, rocket launches, stargazing, and entertainment tied to the stars. If you read about it on Space.com last week, it might just show up in this puzzle. And if you didn't? Well, now's your chance to catch up while flexing your trivia muscles.
So channel your inner astronaut, and dive into this week's interstellar quiz. The answers are out there, you just have to connect the clues.
Try it out below and see how well you do!
When learning about the effects of spaceflight on human health, you typically will hear about the dangers of radiation, bone density loss and changes in eyesight. While these long-term risks are important, a less frequently discussed concern is motion sickness.
As a child, one of us (Taylor) was highly prone to motion sickness – whether in the backseat of a car, sitting on a train or riding a bus. At the time, she considered it a cruel twist of fate, but as an adult – and a scientist to boot – Taylor can tell you with confidence that it was entirely her fault.
Sometimes, looking out the side window would help, but more often than not, Taylor's dad would have to pull over at the next gas station for a short break, or else they'd all suffer the consequences.
Now, she understands what was happening on a more fundamental level. As children, you are taught about the five senses: sight, hearing, smell, taste and touch. However, there is a hidden sixth sense that helps your body understand how you are moving – the vestibular system. The brain takes information from all these senses and compares it to what it might expect when moving, based on past experiences.
Optimally, any disagreement between your vestibular senses and your brain’s expectations would be small. But when there are large, sustained conflicts, you get sick.
While reading in the car, Taylor was staring at nonmoving words on a page while her vestibular system told her brain she was traveling down a road. This discrepancy confused her brain since usually, when Taylor felt movement, she should see the world shifting around her in the same way – hence her motion sickness. Had she been looking out the window and watching the world pass by, she would have been fine. Even better, had she been in the front seat, she would have been able to see the road ahead and predict how she would move in the future.
The sensory conflict between what you experience and what your brain expects doesn't cause only carsickness. It is also the leading suspect behind cybersickness from using virtual reality headsets, seasickness on ships and spaceflight-driven motion sickness. Our team of aerospace engineers is particularly interested in the latter.
To date, all astronauts have grown up on Earth. So, their brains expect any motion cues to include the presence of Earth's gravity. But when they get to orbit in space, that is no longer the case.
When in orbit around Earth in microgravity, the vestibular system does not have any gravitational input. The conflict between the brain's expectation of Earth’s gravity and the reality of no gravity causes space motion sickness.
Thankfully, the brain's expectations can change over time, after enough exposure to a new environment. Often referred to as "getting your sea legs" in the nautical community, astronauts also eventually overcome space motion sickness while in space. However, overcoming it introduces another problem when they return.
If an astronaut's brain expects microgravity, what happens when they come back to Earth? As you might expect, the process starts again, and astronauts are now prone to terrestrial readaptation motion sickness. To make matters worse, since the retirement of the space shuttle, crew vehicles frequently land in the water, which means astronauts may deal with choppy waves until their capsule is recovered. Seasickness can potentially exacerbate terrestrial readaptation motion sickness.
These conditions are not rare. Over half of all astronauts experience some symptoms of space motion sickness when they first get to space, and terrestrial readaptation motion sickness occurs at a similar incidence rate when they come back down.

If you have ever experienced motion sickness, you know how hard it is to do anything other than close your eyes and take deep breaths to expel the creeping urge to vomit. As a passenger in a car, that may be OK, since you aren't expected to jump into action at a moment's notice. But while isolated on the water in a return capsule, astronauts need to remain focused and clearheaded. In case of an emergency, they'll need to respond rapidly.
If the astronauts need to get out of the capsule prior to pickup up by the recovery team, any motion sickness they have could delay their response time and impede evacuation attempts.
Presently, most astronauts rely on medication that interrupts the brain's ability to use hormones to trigger motion sickness. However, as with many commercial products, these drugs can cause side effects such as drowsiness and can lose efficacy over time.
Our research team completed two experiments to investigate how we might be able to manipulate visual information to mitigate motion sickness in astronauts, without relying on pharmaceuticals.
Our participants were exposed to motions meant to simulate transitions between gravity environments and then ocean wavelike motion. During the hour of wavelike motion, we investigated whether a "virtual window" could reduce the incidence of motion sickness.
When in a capsule on the ocean, astronauts are strapped into their seats and likely cannot see out of the small windows built into the capsule. In place of windows, we used virtual reality headsets to create a full-view virtual window.
In our control group, the subjects received no visual cues of motion – akin to Taylor's poorly advised backseat reading. Meanwhile, one countermeasure group got to see a visual scene that moved naturally with their motion, like looking out the side window of the car at the surrounding world. The other countermeasure group saw a scene that moved appropriately and was provided an overlay showing future motion, like looking out the front window and seeing the road ahead.
As expected, the group with no cues of motion got the sickest. Two-thirds of the subjects needed to stop prior to finishing an hour of wavelike motion, due to excessive nausea. Only about one-fifth of the group that was given the side window view needed to stop early. Only one-tenth of the front window group that received present and future visual cues dropped out.
These results mean that by tracking the capsule motion and projecting it on a headset for the astronauts inside, our team may be able to reduce debilitating motion sickness by roughly half. If we could figure out how to predict how the capsule would move, we could give them that front window experience and improve the landing even more. In case of emergency, they could always take off the headsets.
This work shows promise for motion sickness interventions that do not rely on pharmaceuticals, which are currently used to combat these effects. Our solutions don't have the same concerns around shelf life, stability or side effects. In addition to the benefits for astronauts, such approaches could help those prone to motion sickness here on Earth, particularly in scenarios where looking out the front window at the road isn't feasible, such as on planes, trains, buses or high-speed transportation.
This article is republished from The Conversation under a Creative Commons license. Read the original article.
]]>On Episode 185 of This Week In Space, Rod Pyle and Tariq Malik are joined by Josh Dinner to discuss NASA's Goddard Space Flight Center future, given it is in the administration's crosshairs.
With cuts to their budget and staffing beginning under Elon Musk's DOGE, it has taken a different form with the government shutdown. Employees furloughed or retired from critical programs, laboratories shuttered, and entire facilities gutted — all without the approval of Congress. By the time the shutdown is over, NASA's primary research center — and the one most responsible for what many are now calling "the C-word," climate science — will be a shell of its former self. Dinner recently completed a months-long investigative report.
Also: Jared Isaacman is back in the running as NASA chief, the 25th anniversary of the ISS, and China now working with the US on orbital dangers.
Download or subscribe to this show at: https://twit.tv/shows/this-week-in-space.
Get episodes ad-free with Club TWiT at https://twit.tv/clubtwit

Looking for a telescope to see planets and comets? We recommend the Celestron Astro Fi 102 as the top pick in our best beginner's telescope guide.
Finally, did you know you can launch your own SpaceX rocket? Model rocket maker Estes' stunning scale model of a Falcon 9 rocket that you can pick up now. The launchable model is a detailed recreation of the Falcon 9 and retails for $149.99. You can save 10% by using the code IN-COLLECTSPACE at checkout, courtesy of our partners collectSPACE.com.
This Week in Space covers the new space age. Every Friday we take a deep dive into a fascinating topic. What's happening with the new race to the moon and other planets? When will SpaceX really send people to Mars?
Join Rod Pyle and Tariq Malik from Space.com as they tackle those questions and more each week on Friday afternoons. You can subscribe today on your favorite podcatcher.
]]>Camera specs are thin on the ground but it's 12MP and features a 2-axis gimbal for tilting the camera, which is supported by Electronic Image Stabilization (EIS) rather than the more effective mechanical stabilization that's delivered by 3-axis gimbals. It certainly smooths video, but it can't eliminate larger movements of the drone during flights.
Weight: 8.78 oz / 249 g
Dimensions: : 5.5 x 3.5 x 2.17in / 140 x 90 x 55mm folded / 8.37.1 x 2.17in / 210 x 180 x 55mm unfolded
Battery: 2000 mAh Li-ion / up to 30 minutes flight
Charger type: USB Charging hub
Modes: Camera, Normal, Sport
Video transmission range: 3.7 miles
Video resolution: 4K, 720p (720p stored on phone)
Frame rates: 4K 30FPS stored on microSD / 720p 30FPS stored on smartphone
This produces FPV-style video footage where the tilt pitch and roll of the drone are captured to produce a more immersive type of video. This isn't for everyone, but if you'd like this type of video capture, the HS360E could be one of the best beginner drones for you. Video is captured at 4K 30 FPS on the microSD card in the drone, while 720p 30FPS video is captured on your smartphone with the HS Fly app installed.
Photos are captured in JPEG format in either 4000 x 3000px or 3840 x 2160px (4K) dimensions on the microSD card. Photos saved to your smartphone are in 4K dimensions. Image quality isn't the best but we'll cover that in more detail later. Several features are great for beginners and these include GPS Return to Home, subject tracking, timelapse, panorama, slow-motion video and several automated flight patterns.

The HS360E, as previously mentioned, looks similar to the DJI Mini 4K with its light gray airframe and folding design. The propeller arms fold out horizontally, which takes it from 5.5 x 3.5 x 2.17in / 140 x 90 x 55mm when folded to 8.37.1 x 2.17in / 210 x 180 x 55mm when unfolded, with a weight of 8.78 oz / 249 g. This means that US pilots won't have to register the drone with the FAA if flying recreationally.
The overall design is simple, but the build quality is good. The overall kit looks and feels like good value for money. There are no sensors on the drone for collision avoidance, but there is a much more basic optical flow sensor facing downwards on the bottom of the airframe.
There is also a light on the bottom that changes color to signify whether or not the controller is connected. In low-light conditions, the light on the bottom of the drone could allow the pilot to identify the orientation of the drone. In daylight, it's impossible to see once the drone is in the air.






The HS360E gimbal is extremely simple with only a 2-axis movement for changing the tilt of the camera, with smoothing of video provided by Electronic Image Stabilization. The tilt mechanism of the gimbal isn't the most refined — it's difficult to position it between -90 and 0 degrees and easiest to either set the camera to look forward or straight down.
The 2000 mAh Li-ion batteries are advertised to provide up to 30 minutes of flight. During testing, flight times were coming in at around 19 minutes before a low battery warning came on. This was in 50°F / 10°C temperatures, so during the summer, it's safe to assume that this would increase slightly but certainly not to 30 minutes. So, with only one battery in the kit, a second and possibly even a third would be a worthwhile investment.


The controller that comes with the HS360E is the most common controller with Holy Stone drones and it looks like it's heavily inspired by the DJI RC-N2 controller, but with a basic screen to show flight information. Build quality is lower than the DJI RC-N2, but it's not bad either and it's comfortable to hold and easy to operate, which is most important.
There's a telescopic phone holder at the top where the phone cable can be stored and the control sticks can be unscrewed from the gimbals and stowed in rubberized compartments at the bottom of the unit.
Where most of these controllers come in dark gray to match Holy Stone drones that are typically this darker tone, this version comes in light gray to match the HS360E. There are seven direct access controls to make operation more convenient.

The HS360E uses the same Holy Stone app as the higher spec and more expensive Holy Stone HS600D; the features and functionality of the two drones are extremely similar, despite the HS360E being the more basic model of the two.
The HS360E does fly well and the flight controls are responsive, allowing for smooth operation of the drone to achieve a range of maneuvers, so no complaints here. It's not the fastest and most powerful drone, with a maximum wind resistance of just 12.3 mph, making it unsuited to windy conditions.
This is a GPS-enabled drone like most, if not all, consumer camera drones. This holds the drone in a hover so it doesn't get blown along in the wind. Although, there is both vertical and horizontal movement of the HS360E to the extent that it's best to keep a close eye on the drone when hovering at lower altitudes. With no collision avoidance, this drifting could result in a collision but is, of course, much less of an issue when flying at higher altitudes.
GPS also allows for GPS Follow Me, which uses the GPS signal from your smartphone to track you. This works reasonably well but it's far from the most sophisticated application of the feature. GPS also delivers Return to Home (RTH) functionality with Smart RTH to return the drone to the take-off point at the touch of a button. Return to Home also offers Failsafe RTH and Low Voltage RTH, which return the drone when the signal to the controller is lost or when the battery charge is low.
RTH is both a functional and safety feature that can be extremely useful in a range of situations, as the feature's application suggests. This, alongside the take-off and landing button on the controller, makes it safe and easy to get the drone up and into the air.
This button also initiates an emergency stop when depressed for two seconds, but this only works when the drone is below 16 ft. Then there's Optical Flow Positioning for indoor flights when a GPS signal is unavailable.
The HS360E also offers shooting modes including Panorama, Time-lapse and Slow Motion video. These are easy to use and certainly provide some creative options for beginner pilots. One point to make concerning panoramas is that these are saved to your smartphone, rather than the microSD card, and that they're captured at such low pixel dimensions that they're only suitable for web use.
Within the Multi-functions menu, there are automated flight patterns available, including Point of Interest, Catapult, One-key Ascension and Spiral Up. AI Subject Tracking is a feature where you draw over the desired subject in the HS Fly app and the HS360E camera follows the selected subject effectively. The drone remains in a hover, so you have to fly it to maintain tracking of moving subjects. Other options within the menu include VR capture, Gesture Selfie, Selfie Video and Camera Filter.
Camera specs are thin on the ground, but we know that the camera has a 12MP sensor. This can capture photos in JPEG format in either 4000 x 3000px or 3840 x 2160px (4K) dimensions on the microSD card in the drone. Photos saved to your smartphone are in 4K dimensions. Video is captured at 4K 30FPS on the microSD card, while 720p 30FPS video is captured on your smartphone.
The camera itself is automatic, so you simply point and shoot to capture photos and videos. The only adjustments available are for white balance, contrast, saturation, sharpness and brightness, so there is some control available but it is limited. The exposure of the automatic camera is pretty good and if you find it's too light or too dark, it can be adjusted using the brightness control.

One issue with the camera only having a 2-axis gimbal for tilting the camera while relying on EIS to smooth video, is that the pitch of the drone is captured when you first fly forwards or backwards. Any movement of the drone is captured in videos with the EIS removing only vibration. This produces an FPV look in videos. To combat this to a degree, flying slowly and smoothly does reduce the pitch and roll of the drone, so it's less prominent in videos.
For photos, the roll of the drone into the wind when hovering can result in the horizon being captured at a 45-degree angle. Image quality from the automatic camera is on the soft side and JPEG processing is visible in photos. Video quality is better, as is often the case with drones, and videos shot in brighter conditions typically look best. This does mean that it's not the best drone at this price point for camera functionality.






The Holy Stone HS360E costs $249 / £269. This is a good price for a beginner drone in the sub-250 g category but the HS360E faces some stiff competition from several manufacturers.
The HS360E comes in a kit that includes the drone, a controller, one battery, a charging hub, phone connection cables, a USB-C cable for battery and controller charging, a spare set of propellers and a shell case with a shoulder strap to carry everything. The case offers two cutouts for batteries but I think it would be worth purchasing a second battery to increase flight times.
The HS360E is a basic drone with a point-and-shoot camera that relies on Electronic Image Stabilization to smooth video, which produces a more FPV style of video capture. It does fly well and features available include time-lapse, slow-motion video, panorama and GPS subject tracking, so you do have creative options available.
Build quality is good and the HS360E is undoubtedly easy to set up and use. The size and weight of the drone are also ideal for beginners. However, if you'd prefer a drone with a more advanced camera and gimbal functionality, this isn't the drone for you.
The Holy Stone HS900 is the best Holy Stone drone available and is also a sub-250 g model. It offers excellent flight capabilities and a high-quality camera for capturing photos and videos.
The DJI Mini 4K is DJI's most basic sub-250 g drone that's capable of capturing 4K video and Raw photos. It flies incredibly well and benefits from DJI build quality and overall performance.
The DJI Flip is a selfie drone with camera drone functionality. This means it can track you intelligently or you can fly it yourself to capture aerial photos and videos. Plus, it features built-in propeller guards.
]]>Despite our inability to find aliens (yet!) in our own extraterrestrial searches, our favorite movies, TV shows, games, and books often depict the cosmos as a nightmare realm teeming with horrors, from hostile alien intelligences to races of hive-minds desperate for conquest (or just the sweet taste of human flesh).
Like terrestrial monsters, evil aliens are often stand-ins for real-life anxieties. So, we've steered our list towards those races that are also metaphors for terrors we grapple with here on earth, be it fear of the other or the terror of the unknown. Grab your pulse rifle, and maybe a shotgun for close encounters, because these are the scariest aliens ever conceived.

We tried to avoid putting them on the list, but resistance was futile; it's The Borg. Star Trek's collective race of assimilating monstrosities is so terrifying because they represent the loss of our individuality. An ever-adapting fusion of flesh and technology, the Borg are a hostile force that seeks not just to eradicate humanity, but to enslave it, forcibly eradicating the sense of self and folding its victims into a homogenous hive mind.
Death is scary, but the kind of ego death inflicted by the Borg is arguably a fate worse than death. The implication is that you continue to exist, perhaps even conscious on some level of what you've lost, while everything that defines you is annihilated. The Borg represent our fear of erasure, of disappearing into a vast, flat, and uncaring bureaucracy, and are one of modern fiction's most deft updates to the existential horror first popularized in the fiction of Franz Kafka.
Also, they've got big cubes, the most horrifying of the geometric shapes.

While the xenomorphs are the real OG of alien monsters, and likely the first thing you thought of when you clicked on this list, Alien Earth has introduced an even more horrifying creature to the Alien franchise. If you haven't seen the show, the T. Ocellus is an abominable little beast that resembles an eyeball (or pod of eyeballs) atop an octopus-like body of super-strong tentacles.
The presentation is scary enough, but the real horror is Ocellus's ability to take over a host. It burrows in and replaces one of its victim's eyes, then extends its prehensile tentacles throughout the host's body to take over the host's motor functions. It combines the worst features of face huggers, zombies, and incomprehensible alien horror into a single, compact atrocity.

The Warhammer 40K universe is full of alien and demon threats to humanity, but one of the most vile and terrifying is the Tyranids, the race of extragalactic swarm organisms that have invaded our galaxy to devour all biomass.
They come in their countless billions to overwhelm the advanced weaponry of other species with their sheer numbers, and consume everything in their path like a host of evil, muscled, powerful alien locusts.
The Tyranids represent man's fear of the natural world, nature's inexorable ability to overwhelm, decay, and devour all of man's greatest works. Like the vast, uncaring jungle in Joseph Conrad's Heart of Darkness, the Tyranids are an irresistible force that seeks to surround and destroy humanity through the weight of pure biological necessity. Also like the natural world, the Tyranids are patient, slowly devouring the edges of the galaxy and reproducing in unthinkable numbers in the darkness of space.

One of film's best representations of paranoia, The Thing works on a number of different levels. An alien organism that can perfectly mimic another creature, its ability to duplicate a person's speech, mannerisms, and absorb their memories makes it a perfect analog for the deep-seated human fear of the other, and our inability to trust any entity outside of our direct control.
The Thing builds tension based on the premise that anyone, even your closest friend or partner, could be othered, transformed into a being that longs for your destruction. By subverting trust and building paranoia to screeching highs, The Thing exploits some of humanity's worst traits.
It's a perfect example of a filmmaker (in this case, John Carpenter at the peak of his powers) using an alien being as a lens to demonstrate how humanity's worst enemy will always be its own negative impulses.

While many commonly think Pennywise from Stephen King's "It" is a demonic clown, in reality, it's an ancient, trans-dimensional, malevolent entity that is billions of years old. It assumes the form of a clown on earth in an attempt to lure children, but Pennywise's true nature is much scarier and unknowable.
Pennywise is from a void that exists outside our dimension called the Macroverse. It arrived on our planet many millions of years in the past, and hibernates beneath the town of Derry, Maine, awakening once every 27 years to sate its dark hunger.
Worst of all, Pennywise exploits our most primordial terror, our fear of fear itself, presenting its victims with bloodcurdling illusions to "salt the meat" with dread.

When a barren couple discovers a crashed alien spacecraft housing a small child, they believe their prayers have been answered. As the child develops, however, and his darkest impulses begin to surface, they realize that what they've discovered is a curse cloaked as a blessing.
Brightburn works because of how it inverts several popular tropes and preconceptions. First and foremost, there's the superhero trope, and very specifically the Superman mythos, where we expect the farm-raised, super-powered alien to become humanity's savior (rather than its scourge).
Even more poignant, however, is the Rosemary's Baby angle, where the innocence of childhood is drowned in blood and the notion that a young person reared in a loving environment should develop into a compassionate adult is perverted into unthinkable horror. Brightburn also twists the family dynamic to expose a parent's worst fear, that their power and authority over their children is completely illusory.

One of the most underrated sci-fi horror films of the mid-2010s, Dark Skies tells the story of a struggling American family terrorized by an intergalactic menace. It begins by preying on our fear of the unknown: household goods are arranged in strange patterns, birds commit suicide by crashing into the family's home, and the children begin to suffer nosebleeds and missing periods of time. The family is driven to a state of frenzied paranoia before the threat is revealed, spindly grey aliens that stand above them at night as they sleep.
Dark Skies does an excellent job of using an alien threat as a metaphor for the pressures on the nuclear American family that lead to so many of them disintegrating. The film begins with marital and financial stressors and exacerbates them with the influence of predatory external forces. It's also expert at showcasing a parent's fear of their inability to protect their children in a dangerous and hostile world, and the terror of a safe space like a suburban home being shattered by implacable forces beyond our control.
]]>Jupiter is currently situated against the stars of Gemini the Twins where the ecliptic — the apparent path of the sun, moon and planets — comes farthest north, at +23 degrees declination. This is fortunate for Northern Hemisphere observers, since the farther north a planet is, the more time it will spend above the horizon and the higher it will stand above the southern horizon at the midpoint of its path across the sky. For those living in the southern U.S., when Jupiter crosses the meridian in the early morning hours, it is not far from the point directly overhead (the zenith).
In fact, if you look about 3.5 degrees to the upper left of the moon, you'll see a bright star. It will not be as conspicuous as Jupiter; in fact, it will shine only about 1/28 as bright. Nonetheless, at first magnitude it ranks among the 21 brightest stars in the sky. That star is Pollux, the brightest star of Gemini. Pollux marks the head of one of the twin brothers, the head of the other brother (Castor) can be found almost directly above Pollux.
Because the moon appears to move to the east (left) against the background stars at roughly its own apparent diameter each hour, its position relative to Jupiter and Pollux will change noticeably during the course of the night.
The time when all three objects are more-or-less aligned along a straight line; when the moon appears to sit directly between Pollux and Jupiter, will differ depending on where you are located.
Those in the Eastern time zone will see this happen within a few minutes of 1:45 a.m.
For those living within the Central time zone, this will happen at around 12:25 a.m.
In the Mountain time zone the line-up comes at approximately 11:20 p.m. and for those in the Pacific time zone, only shortly after the moon, star and planet have risen: around 10 p.m., very low above the east-northeast horizon.
If you cast a gaze toward the moon as dawn breaks on Monday morning, note how much the configuration has changed; the moon has moved well off to the east leaving Jupiter and Pollux behind.
Jupiter is currently the best observer's planet and will remain so all winter and into next spring. But sharp telescopic views are seldom possible until it is about 30 degrees above the horizon, given the typical turbulent state of Earth's atmosphere. You'll have to wait until midnight for Jupiter to reach 30 degrees altitude, which to some is the psychological dividing line between objects that are "low" and "well placed." Half the area of the hemispherical sky dome is below 30 degrees altitude (or "three fists").
If you do check out Jupiter with a small telescope on Sunday night, you'll see all four Galilean moons, with Ganymede and Io on one side of Jupiter and Europa and Callisto on the other. The ever-changing positions of the satellites relative to each other are always fun to watch.
Joe Rao serves as an instructor and guest lecturer at New York's Hayden Planetarium. He writes about astronomy for Natural History magazine, Sky and Telescope and other publications.
]]>Scientists use TESS to hunt for extrasolar planets, or "exoplanets," by observing the dips in starlight they cause as they cross or "transit" the face of their star from its viewing angle around Earth. Beginning with almost half a million planetary systems, a team of researchers worked this down to a sample of 15,000 possible planetary signals detected by TESS. The team then applied a computer algorithm that helped them identify only those planet candidates that orbit stars just beginning to become red giants, finding the number to be around 130, including 33 that were new candidates detected for the first time.
This revealed that planets are much less likely to be found orbiting close to a red giant star, implying that many planets get wiped out when their stars undergo the transformation into a red giant.
"This is strong evidence that as stars evolve off their main sequence, they can quickly cause planets to spiral into them and be destroyed. This has been the subject of debate and theory for some time, but now we can see the impact of this directly and measure it at the level of a large population of stars," Edward Bryant, team member and University of Warwick researcher, said in a statement. "We expected to see this effect, but we were still surprised by just how efficient these stars seem to be at engulfing their close planets."
Stars become red giants when they reach the end of the hydrogen in their cores, meaning this lightest element can't continue to be converted into helium, the nuclear process known as fusion that powers so-called "main sequence" stars like the sun. When this happens, the cores of these stars start to contract, but the outer layers, where hydrogen is still transformed to helium, "puff out," causing the star to expand to as much as 1,000 times its original size. That marks the end of the main sequence phase and the beginning of the red giant stage of a star's life.
Obviously, this is bad news for the planets orbiting close to this transforming star. For example, when the sun enters its red giant phase in around 5 billion years, it will expand to swallow Mercury and Venus, and possibly even our own planet. However, this isn't the only method of destruction that this team thinks stars employ as red giants.
"We think the destruction happens because of the gravitational tug-of-war between the planet and the star, called tidal interaction. As the star evolves and expands, this interaction becomes stronger," Bryant continued. "Just like the moon pulls on Earth’s oceans to create tides, the planet pulls on the star. These interactions slow the planet down and cause its orbit to shrink, making it spiral inwards until it either breaks apart or falls into the star."
This is reflected by the fact that when the team focused on stars that had already begun to expand, there was only a 0.11% chance of them hosting a planet. That is around 3% lower than the chance of a main-sequence star hosting a planet. The researchers also found that the chance of a red giant hosting a giant planet such as Jupiter or Saturn also fell as the age of the star increased.
But what does this tell us about Earth's chances of surviving the sun's metamorphosis into a red giant?
"Earth is certainly safer than the giant planets in our study, which are much closer to their star. But we only looked at the earliest part of the post-main sequence phase, the first one or two million years of it – the stars have a lot more evolution to go," Vincent Van Eylen, team member and University College of London researcher, said. "Unlike the missing giant planets in our study, Earth itself might survive the sun’s red giant phase. But life on Earth probably would not."
The researchers will now search for more data in order to better understand why some planets become prey for elderly stars and others do not, which could answer questions about Earth's potential survival.
"Once we have these planets’ masses, that will help us understand exactly what is causing these planets to spiral in and be destroyed," Bryant concluded.
The team's research was published in the October edition of the Monthly Notices of the Royal Astronomical Society.
3I/ATLAS was first discovered in July. It made its closest pass to the sun on Oct. 30, and three sun-facing spacecraft collected images of the wanderer as it zoomed past our star. This imagery revealed that 3I/ATLAS underwent a "rapid brightening" that exceeds what is observed in most comets at similar distances to the sun. In a pre-print study of that imagery published on arXiv, scientists wrote that this new data shows 3I/ATLAS is "distinctly bluer than the sun" in contrast to "earlier observations showing the comet's dust to be red." Numerous media outlets jumped at the chance to declare the comet had "changed color" multiple times and, of course, said it happened for mysterious reasons.
But according to one of the scientists behind this new study, that's incorrect. "We don't have any evidence for the gas coma changing colors," Qicheng Zhang, a postdoctoral fellow at the Lowell Observatory in Arizona and one of the authors of the study, told Space.com by email. "Our result just showed that the gas coma is likely still around and contributing substantially to the overall brightness," Zhang added.
Comets are sometimes referred to as "dirty snowballs" due the fact that their icy solid cores, or nuclei, are made of frozen gases containing bits of rock and dust. As comets approach the sun, these frozen gases turn from solids back into a gaseous state, creating bright haloes of gas known as "comas" that give comets a fuzzy appearance. A coma can also form a long, bright tail as the solar wind pushes these gases away from the comet's nucleus.
Zhang said that, technically, comet 3I/ATLAS has only appeared to "change color" a single time — when its coma became bright as the comet ejected gases while warming up in the sun's heat earlier this year. This was far before reports started emerging about the interstellar visitor's supposed newsworthy "color change."
"As far as we know, the comet just 'changed color' once when its gas coma first became visible/bright, and it's still like that now (only brighter)," Zhang said.
"However, this was already beginning to happen by early September before it got too close to the sun in the sky, as there are numerous photos from amateur astronomers from around then already showing that the comet has a blue/green gas coma."

The comet has been the target of quite a bit of misinformation and extreme speculation, including conspiracy theories that allege it is actually an alien spacecraft and that the U.S. government is using the current government shutdown to conceal evidence of its true nature.
But such extreme circumstances aren't necessary to have this object be as fascinating as it is. Its serendipitous pass through our corner of the cosmos offers us a rare peek into what conditions might be like outside the solar system.
Numerous ground-based telescopes have captured images of the comet, even consumer-grade telescopes as small as 6 inches, and so have the Hubble Space Telescope, Europe's ExoMars Trace Gas Orbiter and China's Tianwen 1 Mars probe.
NASA's Mars Reconnaissance Orbiter was due to capture imagery of the comet as it passed by the Red Planet around Oct. 3, but due to NASA's operations being largely on hold due the shutdown, no imagery has been released from that flyby.
Comet 3I/ATLAS will make its closest approach to Earth on Dec. 19, when it will pass us at a distance of some 167 million miles (270 million km).
]]>But that hasn't stopped Texas-based Celestis, Inc. from launching a new reservation list for customers to stake out coveted spots on the memorial spaceflight company's first planned journey to Mars. Celestis aims to send canisters containing cremated ashes and DNA samples of the deceased into orbit around the Red Planet.
However, it might be an endeavor several years in the making.
Since 1997, the Houston-headquartered firm has carried precious cargo of the remains of loved ones, pets, and luminaries beyond Earth on a number of missions employing a wide range of launch vehicles, most recently United Launch Alliance's new Vulcan Centaur rocket. Other services offered are liftoff and recovery options that are paired with ocean splashdowns in which clients can send memorial capsules into orbit that are then retrieved to be retained as heirlooms and keepsakes.
Now, Celestis has officially opened reservations for the first 300 participants aboard their ambitious Mars300 project. This mission aims to liftoff as a secondary payload for a future, yet-to-be-named Mars-bound cargo spacecraft.
Celestis says the service will cost $24,995, and is already taking 10% down payments for families to reserve a place among the first members of our species to reach Mars. According to a press release, "participant payments will be held in a dedicated, bank-maintained, federally-insured trust account under the client's control until the launch date and provider are confirmed."
According to Celestis Founder and CEO Charles Chafer, his company is looking at 2030 for the first mission. A reliable launcher is obviously still a detail to be determined as currently the only significant provider that might be offering cargo odysseys to Mars is SpaceX’s Starship.
"This mission represents humanity’s next responsible step toward the stars," said Chafer. "By sending cremated remains and human DNA to Mars, we unite science, exploration, and legacy in a way that speaks to our shared destiny beyond Earth."
Questions remain regarding this enterprise, but Celestis’ has stated that its primary goal is to honor loved ones while preserving Mars’ delicate ecosphere through strict adherence to COSPAR planetary protection protocols. Precisely how rigorous planetary protection standards will be enforced is also something to consider.
Longer missions into the great beyond have included cremated remains and/or DNA canisters of "Star Trek" legends like Nichelle Nichols, DeForest Kelley, Gene Roddenberry and his wife Majel Barrett Roddenberry and James "Scotty" Doohan. Celestis also carried symbolic remains belonging to "2001: A Space Odyssey" and "Close Encounters of the Third Kind" VFX legend Douglas Trumbull aboard the 2024 "Enterprise Flight."
This past summer, The Exploration Company's "Mission Possible" Nyx capsule and its Celestis Memorial Flights payload was sadly lost at sea during its Pacific Ocean splashdown phase when a parachute did not properly deploy.
]]>The reason for this underestimate wasn't due to a lack of data, but was a result of how Juno's data was interpreted. The results also demonstrate that about half of the heat radiating from Io comes from just 17 of 266 the moon's known volcanic sources. The team behind this research thinks that this clear concentration of heat, rather than a global emission, could suggest that an Io-wide lava lake may not exist beneath the surface of this moon of Jupiter as has previously been theorized.
"In recent years, several studies have proposed that the distribution of heat emitted by Io, measured in the infrared spectrum, could help us understand whether a global magma ocean existed beneath its surface," team leader Federico Tosi of the National Institute for Astrophysics (INAF) said in a translated statement. "However, comparing these results with other Juno data and more detailed thermal models, we realized that something wasn't right: the thermal output values appeared too low compared to the physical characteristics of known lava lakes."
Tosi continued by explaining that until now, studies of Io have focused heavily on a specific band of infrared light known as the M-band. M-band data collected by the Jovian InfraRed Auroral Mapper (JIRAM) aboard Juno have been invaluable in identifying the hottest regions of Io and thus for understanding its volcanism, but Tosi says the measurements collected in this spectral band could have influenced previous heat estimates
"The problem is that this band is sensitive only to the highest temperatures, and therefore tends to favor the most incandescent areas of volcanoes, neglecting the colder but much more extensive ones," Tosi said. "In practice, it's like estimating the brightness of a bonfire by observing only the flames and not the surrounding embers: you capture the brightest spots, but you don't measure all the energy actually emitted."
Reconsidering their approach to analyzing Juno's JIRAM data changed the team's view of the structure of Io's lava lakes. They found that most of Io's volcanoes are not uniformly hot but instead possess a hot and bright outer ring with a cooler, solid central crust. This latter region is less bright in the M-band of infrared light but covers a larger surface area, allowing it to emit an enormous amount of heat.
"When this 'hidden' component is also considered, the actual heat flux is up to hundreds of times higher than that calculated by analyzing the M-band alone," Tosi continued. "This is a significant leap, because it changes the scale of the satellite's [Io's] energy balance."
This could have implications for the suggested global ocean of magma below the surface of Io, but Tosi is clear that the existence of this feature isn't something that can be completely ruled out by this research. In fact, he theorizes that M-band JIRAM data can't be used to confirm this magma ocean.
"Our caution, therefore, is well-founded: we're not saying that such an ocean doesn't exist, but that it can't be deduced from these observations," Tosi said. "It's important to recognize the limitations of the available data before drawing too strong conclusions on such a complex issue."

Unfortunately, it may be a while before scientists get such a good look at Io again, so the question of its global magma ocean may remain unanswered.
"In 2023 and 2024, Juno performed the closest and most detailed observations of Io ever obtained by a spacecraft. In the coming year, however, the natural evolution of the spacecraft's orbit will not allow for such close passes again," Tosi said. "Future missions to the Jovian system, such as ESA's Juice and NASA's Europa Clipper, will not be able to observe Io with comparable spatial resolution, as they will be primarily dedicated to Ganymede and Europa.
"Nevertheless, monitoring Io remains crucial."
He added that the team's findings should provide a framework that can be used to more accurately interpret even remote spacecraft observations of Io. This could finally help researchers get to the bottom of why this Jovian moon is so violently volcanic.
"Looking ahead, this experience could also inform the design of future missions specifically dedicated to Io, which could finally directly observe the processes that fuel the most intense volcanism in the solar system," Tosi concluded.
The team's research was published on Wednesday (Nov. 5) in the journal Frontiers in Astronomy and Space Sciences.
]]>Price: $149.99 / £119.99
Type: Survival horror
Players: 1-5
Recommended age: 12+
Time per game: 2-3 hours
Complexity: 7/10
The setup is simple. You and up to four other players awaken from hypersleep to find the corpse of an unfortunate crewmate splayed across the floor, with a rather large hole in their chest. From there, your mission is broadly to survive. You'll need to make sure that various ship systems haven't been damaged and make it back into stasis before the ship jumps into hyperspace again, killing anyone who isn't tucked into bed.
Oh, and you'll need to keep an eye on your crewmates because one or more of them might have their own nefarious agenda. Of course, you've usually got bigger problems to deal with, what with the xenomorph menaces running around the ship trying to chop your head off or lay eggs in your chest. So, teamwork makes the dream work, but you'll need to watch your back.

Nemesis is a big board game — it comes in a huge box and it's packed full of highly-detailed miniatures for the player characters and aliens (called Intruders). There's also a double-sided board, loads of room tiles, multiple decks of cards and a mountain of tokens and widgets.
The plastic miniatures are gorgeous and there are loads of them too. Each of the six playable characters gets a mini, complete with a color-coded base rim so you can easily identify where you are on the board. However, the real stars of the show are the Intruders, who come in five different forms of ascending size: Larvae, Creepers, Adults, Breeders and the Queen. The adults are by far the most common, so they have multiple sculpts. All the included minis are stunning and if you want to paint them up yourself, you can make them look even better.


Alongside all that, you get a comprehensive rulebook and a pair of quick reference cards that let you know what you can do in all the various rooms on the ship. Reading that rulebook should be your first port of call before setting up your first game. There's quite a lot going on with Nemesis and the rulebook includes a handy set-up guide explaining everything you need to do before your sci-fi horror adventure gets underway. Everyone chooses a character, gets their starting equipment and a pair of objectives that will appear later in the game.
Each character has unique equipment and abilities. The Soldier is best at fighting, the Captain can order other players about, the Engineer is good at fixing things etc. As a result, your character choice can have a huge impact on how you choose to play the game.

The ship is set up with a randomized room layout (in the game's lore, you all have cryosleep-induced amnesia, which explains why none of you know the layout of your spaceship). The easy "side A" layout is recommended for your first few games, whereas the reverse of the board has an alternative layout for experienced players. You'll also need to shuffle the various decks of cards and keep containers of tokens nearby for things like wounds, fires, broken systems and doors.
From there, you simply place everyone in the hibernatorium and the game begins.

At first glance, Nemesis is quite a complicated-looking game, and while it's true that there are a lot of moving parts and mechanics, it's surprisingly intuitive once you get into the swing of things. Before long, everyone will know when to roll for noise, when to place a token down on the board and what they need to do in their turn.
Nemesis is a mostly cooperative game…Mostly. You see, each player broadly needs to stay alive, and you'll have a better chance of fixing the ship if you work together, but every member of the crew is also given two private objective cards at the outset. One of these is a personal objective, and it's usually fairly benign — send a signal, make sure everyone survives — that sort of thing. The other is your corporate objective, and, in fitting with Alien's core messaging of "giant corporations are bad", these objectives tend to be a bit more devious. You might be tasked with smuggling an alien egg off the ship, getting a specific player killed or even blowing up the ship (jettisoning yourself in an escape pod).

Players don't have to choose an objective until the first alien shows up, but you'll never know which objective your crewmates have chosen. There are more friendly and neutral objectives than truly despicable ones, so odds are that you're all on the same page, but you'll never know for sure.
The game will typically last for 15 turns (around 2-3 hours), assuming the ship and/or players survive that long. If you're not careful, fires, malfunctions and the dreaded self-destruct system can all bring about the demise of the Nemesis long before it reaches its destination.
The ship is made up of a series of rooms connected by corridors, but you won't know which rooms are where until you move into them. Each room has a special action that you can perform there, so it pays to explore the ship early on to find all the key locations — you don't want to be blindly stumbling through the hallways, clutching a bite mark, desperately trying to find the med-bay. Some rooms are in fixed locations, such as the engines and bridge — both rather vital systems that you'll want to make sure are in working order.

At the start of each round, players draw up to five cards. From there, each player takes two actions — things like moving, shooting, etc. — before handing over to the next player. When the action swings back around to you and you can still do more, you get another two actions. Once every player has expended their available moves (or passed), the round ends.
The twist here is that every action has a cost, paid using the cards in your hand. As a result, you're eternally being forced to make sacrifices as you choose which cards to play and which to burn to pay for your actions. Do you want to move into the next room normally and save some resources, or move quietly and throw away that repair card that might come in handy later?
Every time a player moves, they make a noise roll that usually results in leaving a noise token in a corridor. Careful movement costs you an extra card, but it lets you pick where the noise token goes, instead of leaving it to fate. This is often essential, as if you ever have to place a noise token where one already exists, you'll attract the attention of the Intruders.
When someone does make enough racket to draw the attention of the Aliens and the proverbial space poop hits the fan, your best-laid plans will quickly melt away. Aliens range from tiny Larvae that infect you à la Facehuggers, all the way up to the mighty Alien Queen herself, who is more likely to bite your head off. The majority of your time will be spent facing off against Adults — these most closely resemble Gieger's iconic movie monster, and they're just as much of a handful to deal with.

Combat with the Intruders is unreliable and quickly depletes your resources. They can deal serious damage to you in a heartbeat if you're unlucky, so you'll need to make smart choices about whether to burn through your ammo, work together to bring down a beast, or run away and leave someone else to deal with the problem.
Nemesis is a game that forces an unrelenting tide of difficult choices on you. Run-ins with the Intruders can lead to you getting infected, which creates numerous issues for you. Your deck gets gummed up with useless infection cards, reducing your effectiveness. If you don't get those infection cards scanned (using the nifty scanner device included in the game) and removed from your deck, they can end up killing you, even after the game has finished.
So do you risk running the gauntlet to the med-bay to treat yourself — and potentially get mauled by Aliens along the way — or do you climb back into your cryo pod and take your chances?



Event cards throw more spanners into the works too, unleashing some form of calamity onto the ship at the end of each round. These can break systems, start fires, lock doors or even trigger the self-destruct system, while also potentially causing Intruders on the board to move to adjacent rooms.
The first player to be eliminated can even take control of the Intruders if they want, turning on their former allies.
And then there are the other players — can you trust them? Someone checked the engines and said they were working fine, but they've been acting suspiciously and heading toward the escape pods for the past few turns. Maybe they're just heading to the nearby armory to reload their guns, but maybe they're a no-good, double-crossing son-of-a-gun.

Even when you are all working together, there's no guarantee of success (or to put it another way, "I can't lie to you about your chances, but you have my sympathies"). I've died more often than not playing Nemesis. Escaping the nightmare requires you to complete your objective, set the ship's destination correctly, have two of the three engines functioning, avoid too many fires or malfunctions and then either enter the hibernatorium or an escape pod.
That's a lot of things to juggle while biomechanical nightmares are trying to give you a fashionable new torso piercing. Mess any of these things up and it's game over.
Almost everyone I've ever played Nemesis with has instantly been clamoring for another go — it's a real story-generating machine. There was the game where our soldier went out in a blaze of glory fighting the Alien Queen, while the cowardly scientist was munched in his own lab, trying to smuggle out an egg. Another time, the escape pod I was running to malfunctioned and jettisoned as I reached the door, leaving me to watch in horror as my chances of survival faded. No go is ever the same.

If you like big board games, Nemesis is an easy recommendation for me as it's probably my favorite board game of all time. There's a lot going on and that can be intimidating for new players, but it's shockingly intuitive, and after a few turns, it all falls into place.
There are always choices for the players to make, and there's a ton of variety and replayability thanks to the varied objectives, randomized ship layouts and chaotic nature of the game.
Yet it's the co-op-ish nature of Nemesis that elevates it to gaming greatness for me. There are plenty of traitor games out there but Nemesis does something more with it. Everyone could be working together but you don't know if there is someone out to screw you over, and this creates a delightful undercurrent of paranoia throughout the whole game.
It might be lifting a lot of its inspiration from Alien, but it nails the tone and messaging of the universe. Alien was the perfect organism, but Nemesis is the perfect Alien board game.
If you like the sound of Nemesis, but don't want to invest in such a heavy-duty, expensive board game, then you should absolutely check out Alien: Fate of the Nostromo. Ironically, it's just a simplified version of Nemesis. It's the same core experience with a lot of the crunchy details streamlined away, and it's an actually licensed Alien game, so you get to play as Ripley and the Nostromo crew!
The Captain is Dead is also a stellar option. It's a 2 to 7-player game where you must all work together (no sneakiness here) to defend your spaceship from attacking aliens whilst trying to get the Jump Core back online. The fun, colorful artwork alongside the easier gameplay, making for a shorter playing time (60-90 mins), means this space board game would suit those newer to strategy board games as well as a younger audience.
Finally, you could also go digital and enjoy some of the best Alien games of all time.
]]>One of Saturn's moons, Enceladus has been known to be an active ocean world ever since 2005, when the Cassini mission found giant plumes of water vapour squirting up from the ocean deep below through huge fractures in the surface. These plumes are powered by energy from tidal interactions with Saturn, which flex the moon's interior, subtly squeezing and stretching it and ultimately keeping its interior warm enough for liquid water.
The question of how long Enceladus' ocean has existed is an unanswered one, but with water, heat and the right organic chemistry for life, Enceladus is viewed as a prime target for the search for life beyond Earth.
"Enceladus is a key target in the search for life outside the Earth, and understanding the long-term availability of its energy is key to determining whether it can support life," said study leader Georgina Miles, of the Southwest Research Institute and a Visiting Scientist at the University of Oxford, in a statement.
If Enceladus didn't continually receive enough energy from tidal heating, its ocean would gradually freeze. If it received too much energy, the activity in the ocean would increase, altering its environment perhaps to the detriment of its habitability. Therefore, a careful balance between the energy deposited into the moon by the tidal interaction, and the energy that leaks away through convection up to the surface and into space, is required to ensure stability over hundreds of millions or even billions of years.
Planetary scientists know that heat flows out from the south pole, where the fractures, known as tiger stripes, that produce the plumes are located. However, they thought that Enceladus' north pole was inert.
It seems that they were wrong.
By comparing measurements from Cassini's Composite Infrared Spectrometer (CIRS) of the temperature of Enceladus' north pole during Saturnian winter in 2005 and what passes for summer on the icy moon in 2015, and then comparing it to predicted temperatures based on modeling, Miles' team found that Enceladus' north pole was seven degrees Celsius (45 degrees Fahrenheit) warmer than expected. This excess heat is flowing out from the ocean that is measured to be 12 to 14 miles (20 to 23 kilometers) beneath the surface at the north pole, and averaging 15.5 to 17.4 miles (25 to 28 kilometers) deep globally. This thick ice shell will make it difficult for any future mission to drill down to the ocean; entering via the tiger stripes might be the best bet, even if it might be more dangerous. A mission to launch in the 2040s is currently being considered by the European Space Agency.
The measured heat flow is 46 milliwatts per square meter, which compared to Earth is two-thirds the heat loss through our continental plates. When measured for the entirety of Enceladus, including the heat flow towards the south pole, the moon is losing 54 gigawatts across its entire surface area, which is a close match for the amount of energy that tidal heating puts into the moon. This careful balance is no coincidence, and implies the ocean has been stable, without freezing solid, for a very long time.

"Understanding how much heat Enceladus is losing on a global level is crucial to knowing whether it can support life," said Carly Howett of both the University of Oxford and the Planetary Science Institute in Arizona. "It is really exciting that this new result supports Enceladus' long-term sustainability, a crucial component for life to develop."
Although Cassini ended its 13-year mission in 2017 when it plunged into Saturn to prevent it from crashing onto and contaminating any of Saturn's moons, it seems that the spacecraft is still making discoveries.
"Eking out the subtle surface temperature variations caused by Enceladus' conductive heat flow from its daily and seasonal temperature changes was a challenge, and was only made possible by Cassini's extended missions," said Miles. "Our study highlights the need for long-term missions to ocean worlds that may harbor life, and the fact the data might not reveal all its secrets until decades later after it has been obtained."
The findings were published on Nov. 7 in Science Advances.
As the record-long shutdown of the U.S. federal government stretches into its second month, commercial air travelers are beginning to feel the impacts at the nation's airports. To help ease the strain, the Federal Aviation Administration (FAA) has issued an emergency order to limit who can access navigable airspace, which includes restricted hours on commercial rocket launches.
Beginning 6 a.m. EST (1100 GMT) on Nov. 10, commercial launches to space can only take place between the hours of 10 p.m. EST (0300 GMT) and 6 a.m. EST (1100 GMT), according to the FAA order. This will help keep airspace restrictions in Florida, near NASA's Kennedy Space Center and Cape Canaveral Space Force Station, as well as Vandenberg Space Force Station in California, to a minimum while air traffic delays stack up due to staffing shortages caused by the government shutdown.
Though its impact on greater U.S. air traffic delays across the country will be hard to measure, the restrictions coincide with the busiest coast-to-coast launch cadence in history. The order will primarily affect SpaceX, which routinely launches Starlink satellite stacks into low Earth orbit as it expands its wireless internet megaconstellation, though other launch providers and missions will likely need to reassess their launch manifests. SpaceX has launched over 140 Starlink missions this year alone.
One launch hoping to get off the ground before the order goes into effect is NASA's ESCAPADE mission to Mars. The Rocket Lab-built twin orbiters are scheduled to liftoff on a Blue Origin New Glenn rocket at 2:45 p.m. EST (1945 GMT) on Nov. 9. The impending restrictions mean the ESCAPADE mission won't have a chance to reset for a second launch attempt if the Nov. 9 liftoff is scrubbed for some reason.
United Launch Alliance's Atlas V launch of the ViaSat-3 F2 satellite could face further delays under the new launch restrictions, after two previous mission scrubs earlier this week due to issues with the rocket.
During the shutdown, all federal employees deemed non-essential are furloughed. Those whose job falls into the essential category are still required to go to work, but are not currently getting paid and must rely on backpay once the government reopens.
For NASA, this means nearly 15,000 people staying home from work. That's about 95% of the space agency's workforce. In contrast, 95% of employees at the Transportation Security Administration (TSA) are considered "excepted" and have continued to work without pay since the shutdown began Oct. 1.
.@USDOT has many responsibilities, but our number one job is safety. This isn’t about politics – it’s about assessing the data and alleviating building risk in the system as controllers continue working without pay. It’s safe to fly today, tomorrow, and the day after because… pic.twitter.com/YRrq5sdy4TNovember 7, 2025
In a post on X, Department of Transportation Secretary and Acting NASA Administrator Sean Duffy said the emergency order was, "about assessing the data and alleviating building risk in the system as controllers continue working without pay. It's safe to fly today, tomorrow, and the day after because of the proactive actions we are taking."
]]>Astronomers led by Marta Sewiło of the University of Maryland used JWST's Mid-Infrared Instrument (MIRI) to detect myriad complex organic molecules (COMs) in ice that encase grains of dust around the massive protostar ST6 in the Large Magellanic Cloud (LMC), which is a neighboring dwarf galaxy about 163,000 light years away. COMs are classed as carbon-bearing molecules containing more than six atoms, and many COMs are the chemical precursors to the building blocks of life as we know it.
The frozen COMs that were confirmed to exist around ST6 include acetaldehyde, acetic acid, ethanol, methanol and methyl formate. On Earth, methyl formate and acetaldehyde are used as industrial chemicals, methanol and ethanol are alcohols, and acetic acid is in vinegar. But they are also the backbone of even more complex, "second-generation" molecules that build the likes of amino acids and RNA molecules.
At least another 14 COMs were also detected by JWST, but so far Sewiło and her colleagues have been unable to confirm their identity.
"We have only just started exploring the dependence of complex organic chemistry in this environment," Sewiło told Space.com in an interview.
JWST is breaking new ground in the study of chemistry in environments where stars and, later, planets form.
Stars form when massive clouds of frigid molecular gas begin to fragment and collapse, producing dense cores where stars begin to coalesce. At first, these cores are cold, less than 100 kelvin (i.e., 100 degrees above absolute zero) and complex molecules exist as ices on dust grains. It is only later, when the core grows hotter, that the ice sublimates and releases the COMs as gases.
Whereas COMs in their gas phase have been detected multiple times around young stars in both the Milky Way galaxy and the LMC — for example, both methanol and methyl formate had previously been found in their gas phase around protostars in the LMC — they have been far harder to spot when in the earlier, cold ice phase.
"JWST has enabled the detection of COM ices, but to date there are only four protostars in the Milky Way where we have detected icy COMs, and only one in the LMC — ST6," said Sewiło.
By detecting the COMs in their frozen states, astronomers get an indication of how far evolved the chemistry of the material surrounding protostars is at the earliest stages of star formation.
Their presence around a young, massive protostar in the LMC is also intriguing, given the differing conditions there compared to our Milky Way galaxy. The LMC has properties in common with galaxies that existed when the universe was much younger, namely a lower abundance of elements heavier than hydrogen and helium and a stronger ultraviolet radiation field. The lack of heavy elements could impact the abundance of COMs, while the ultraviolet radiation could affect the rate of chemical reactions.
Therefore, understanding the organic chemistry of the LMC can also help teach us about the organic chemistry of the early universe, in particular how soon the building blocks of life were able to form. This could help place limits on how early, theoretically, life could have formed in the universe.
The dearth of heavy elements in the LMC does seem to have impacted the abundance of COMs around ST6.

"The COM ice abundances with respect to water ice that we measured for ST6 are lower than those measured for the four protostars in the Milky Way for all COMs, as expected, except for acetic acid," said Sewiło. "The overabundance of acetic-acid ice is likely the result of the higher ultraviolet flux in the LMC."
Among the other 14 — at minimum — unknown absorption lines in ST6's spectrum could be glycolaldehyde, which is a chemical precursor to ribose, which is a component of RNA molecules.
"We have found evidence that several of the unidentified absorption features could be attributed to glycolaldehyde, but the detection remains inconclusive since more laboratory spectra are needed to verify it," said Sewiło, alluding to the fact that the star's spectrum is compared to those of different molecules taken in laboratory conditions to identify which absorption lines belong to which COMs.
"It is likely that more COMs are present in the ices around ST6, and our results highlight the need for more laboratory experiments."
As the protostar evolves and heats up, the ice on the dust grains nearest the star will sublimate and the COMs will move into their gas phase, as has previously been detected.
It is in the gas phase that more chemical reactions can take place, triggered by ultraviolet radiation from the protostar and the wider environment, "leading to larger and more complex molecules important for life such as propanol and propanal, and possibly amino acids, but we've not detected them in ST6 yet," said Sewiło.
Amino acids have, however, been found in comets and meteorites in our solar system. Comets and meteorites are ancient bodies, formed 4.5 billion years ago when our sun was a protostar. The implication is that amino acids are the end result of a pathway of chemical reactions that begin with the kinds of COMs discovered around ST6.
The research was published on Oct. 20 in Astrophysical Journal Letters.
Photographers across North America were treated to stunning displays of green, pink, and purple auroras rippling across the sky. We've rounded up some of the best views here.
A G3 geomagnetic storm watch remains in effect through Nov. 8, according to NOAA's Space Weather Prediction Center. Aurora chasers keep those camera batteries charged and those eyes on the skies, as we could be in for more treats this weekend.
Ethan Mok posted this impressive photo of his brother on X. What a hole-in-one!
"I think I just took the hardest golf picture possible of my brother," Mok wrote in a post on X.
I think I just took the hardest golf picture possible of my brother pic.twitter.com/FY4AteGQhmNovember 6, 2025
Photographer Eric Bleicher captured a beautiful timelapse of the northern lights dancing alongside the full moon on Nov. 5.
A short timelapse of the northern lights and the moon pic.twitter.com/pKnNEZpQsINovember 6, 2025
Meanwhile, solar astrophysicist and Space.com contributor Ryan French enjoyed front row seats to the northern lights show while on a flight from Denver to Chicago.
Spotted the northern lights on my flight from Denver to Chicago this evening! pic.twitter.com/XfXBsU0HjINovember 6, 2025
Aurora chaser Landon Moeller spotted the aurora show in the skies above DeKalb, Illinois.
Wow. What a show! DeKalb, IL pic.twitter.com/4rV7iqRlnzNovember 6, 2025
The northern lights were so bright and dynamic they could be captured in good detail in this video from aurora chaser Jeremy Rand.
very fast movement tonight! so pretty pic.twitter.com/VltLZt5vsBNovember 6, 2025
Jason O'Young got a glimpse of the aurora show from Ontario, Canada, despite the full moon and clouds threatening to ruin the party.
"Northern lights visible in Southern Ontario despite the moonlight. This would be ridiculous with no moon out," O'Young posted on X.
Northern lights visible in Southern Ontario despite the moonlight. This would be ridiculous with no moon out. pic.twitter.com/Vg11pvbSStNovember 6, 2025
Senior meteorologist Chris Stammers snapped this lovely aurora display above Winnipeg, Canada.
Insane aurora over Winnipeg right now! pic.twitter.com/qw5g3HXro8November 6, 2025
Editor's Note: If you snap a photo of the northern lights or southern lights over the weekend and would like to share it with Space.com's readers, send your photo(s), comments, and your name and location to spacephotos@space.com.
]]>With its unnerving teasers and trailer that remind those of us of a certain age of uncanny series like David Lynch's "Twin Peaks" and Oliver Stone's "Wild Palms," "Pluribus" remains an enigma wrapped in a riddle to the majority of fans. Its overarching premise of a strange world besieged by a happiness virus and the plight of one immune soul is all we’ve known of the mystery project since first hearing of its development back in 2022.
Now, as the bizarre-yet-enticing series finally launches on Apple TV, we’re here to offer what scant details we’ve collected to deliver a better idea of what to expect from "Pluribus"' peculiar rhythms. Smile and let's begin!

"Pluribus" debuts its first pair of episodes on Friday, November 7, 2025, exclusively on Apple TV.
Subsequent chapters of its intriguing nine-episode premiere season will be released each following Friday. A second season was already approved by Apple TV as part of Gilligan's initial deal.
"Pluribus" is streaming exclusively on Apple TV worldwide. The show is being created in house by Apple, and the streamer has already ordered two seasons.

Watch Pluribus on Apple TV+:
All the debut season of this creepy sci-fi thriller on Apple TV, along with other hit sci-fi shows like Invasion, Severance, For All Mankind, Foundation, and Silo. It's low-key the best streaming service for sci-fi these days.
Apple TV+ costs $12.99 per month, but there is also a free 7-day trial for new members who want to check out the service without committing.View Deal
Out of the country when the show debuts? Not a problem, as you can still watch it on your streaming service of choice using a VPN. You'll be able to connect to the service you've paid for, no matter where you are (on Earth, it won't work in space, sorry).
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Unless you're extremely adept at Scrabble or work as a professional linguist or lexicographer, the vast majority of fans will have only a vague notion of what the word pluribus actually means.
You might recognize the word from "E Pluribus Unum" — the Latin phrase and official U.S. motto seen on American currency. It means "Out of many, one," and signifies how the United States was initially forged via the historic joining together of the 13 original colonies.
Linguistically speaking, pluribus is defined as the ablative plural of the Latin word for plus or more. The title refers to the series' universal optimism pandemic that has somehow swept the planet, creating one unnaturally cheerful global society out of the planet's billions of inhabitants.

Rod Serling's "The Twilight Zone" set the standard for thought-provoking science fiction and fantasy fare back in the 1960s, and Vince Gilligan's "Pluribus" certainly plumbs the depths of the iconic series' core existential themes and examinations of human connections and individuality.
Gilligan has also gone on the record about his "mild" sci-fi show being influenced by 1956's "Invasion of the Body Snatchers" and those hive-minded cybernetic aliens of "Star Trek" known as The Borg.
In "Pluribus", Rhea Seehorn ("Better Call Saul") portrays Carol Sturka, a sad historical romance novelist living in a mundane corner of Albuquerque, New Mexico who is somehow immune to a contentment-inducing virus that's infected humanity. According to the official synopsis, this "most miserable person on Earth must save the world from happiness."
The first cryptic Lynchian-style teasers for "Pluribus" hit the internet this past summer, depicting oddities like people licking donuts and garbage-collecting drones struggling at their job.
A full trailer was released Oct. 22, 2025, that offers a bit more unsettling clues and reveals more of the show's darkly comedic tones. You can see them below:

The signature creative hand responsible for "Pluribus" is executive producer, writer, and showrunner Vince Gilligan, the visionary filmmaker responsible for "Breaking Bad" and "Better Call Saul."
"What interests me about this show and the possibilities for it is that people, I hope, can watch it and say, 'What would the world be like if everybody got along?,'" Gilligan told EW. "There's probably a bit of wish fulfillment in the idea of this show."
As we mentioned earlier, Rhea Seehorn ("Better Call Saul") leads the show as Carol Sturka, a historical romance novelist and apparently the only miserable person left on Earth.
Rounding out the "Pluribus" cast is Carlos Manuel Vesga ("The Luckiest Man in America"), Karolina Wydra ("Sneaky Pete"), Miriam Shor ("American Fiction"), and Samba Schutte ("Our Flag Means Death"). Directors include Gilligan himself, Gordon Smith, Zetna Fuentes, and Gandja Monteiro.

No.
While it comes to us from the same creative minds, and even though it's set in the exact same southwestern U.S. city as those two all-time fan-favorite series, "Pluribus" is set in its own universe and has no connection to the Breaking Bad universe.
There are some connections beyond Vince Gilligan's creative hand, though, as the lead actress, Rhea Seehorn, will be a familiar face to fans of Better Call Saul, as she played Kim Wexler in the show. Pluribus is also set in Albuquerque, New Mexico, just like the Breaking Bad shows and spinoffs.
]]>3I/ATLAS was discovered earlier this year, on July 1, and was swiftly confirmed to be just the third interstellar object known to have visited our solar system. It's believed to have formed around a distant star.
As such, scientists were quick to analyze the comet's light fingerprint using every ground and space-based instrument at their disposal, probing its evolving coma and tail(s) in an attempt to unravel the wanderer's mysteries — and the environment from whence it came.
Now, you can get your shot at laying eyes on 3I/ATLAS, as it emerges out from the glare of our parent star.
Qicheng Zhang, a postdoctoral fellow at the Lowell Observatory in Arizona captured the interstellar interloper with a 6-inch (152-mm) Ritchey–Chrétien reflector through thin clouds in the morning twilight on Nov. 1.
"The comet is now a fairly easy target in the morning for anyone with a camera on even a small telescope with clear skies and a low eastern horizon," Zhang told Space.com in an email. "It currently doesn't look like much, just a blob that's slightly fuzzier than the stars around it, but it should rapidly become more visible (including by eye directly through a telescope) over the next few days/weeks."

Comet 3I/ATLAS can be found travelling amongst the stars of the constellation Virgo close to the eastern horizon in the hours before dawn in early November, with Venus shining brightly beneath. It is currently racing headlong away from the sun on an escape trajectory from our solar system. As the heat radiation from our star decreases, the comet will likely become less visible, though the inherently unpredictable nature of these cosmic nomads makes it difficult to predict when it will disappear from Earth's skies forever.
"If it fades as quickly as it brightened, it'll probably appear visually as its peak in just the next week or two," continued Zhang. "Either way, a telescope (and/or a camera taking long exposures) will most likely be required to spot the comet, barring an unexpected outburst."
Looking to upgrade your gear? Then be sure to check out our roundup of the best telescopes for exploring the night sky. If you're into photography then you might benefit from reading our guide to capturing wandering comets, along with our picks of the best cameras and lenses for astrophotography.
Editor's Note: If you would like to share your images of 3I/ATLAS with Space.com's readers, then please send your photo(s), comments, and your name and location to spacephotos@space.com.
Aboard were 18 payloads, some of them experimental technologies and others satellites, all heading for low Earth orbit. And, like most SpaceX missions, this one featured a rocket landing, which is highlighted above.
Bandwagon is one of SpaceX's two satellite-rideshare programs, along with Transporter. As its name suggests, Bandwagon-4 was the fourth mission in the program, and according to the manifest, it successfully delivered 18 payloads to their target orbits.
This image was taken at Landing Zone 2 at Cape Canaveral Space Force Station in Florida, where the Falcon 9 first stage touched down on Nov. 2.

Rideshare programs make access to space more affordable to various stakeholders that may not be able to afford a dedicated launch, such as universities and start-ups.
These groups can add their experiments and technology to the Falcon 9 rocket — payloads such as Vast's Haven Demo, a pathfinder for Haven-1, a private space station. The successful launch of Bandwagon-4 marks a key step in making space more accessible as humanity continues to look to the stars.
And rocket landings, which SpaceX has made routine over the past decade or so, are amazing in their own right: They help decrease the costs of spaceflight and allow more rockets to get off the pad in a timely fashion.
You can learn more about rideshare missions and SpaceX's work.
]]>Scheduled for liftoff no earlier than Sunday (Nov. 9) aboard Blue Origin's New Glenn rocket from Cape Canaveral, Florida, the $80 million ESCAPADE mission — short for Escape and Plasma Acceleration and Dynamics Explorers — will send two twin probes, nicknamed Blue and Gold, to orbit Mars in tandem. The mission marks NASA's first dual-satellite mission to another planet, and aims to create a 3D view of how the solar wind, the stream of charged particles from the sun, energizes and strips away Martian air.
"To understand how the solar wind drives different kinds of atmospheric escape is a key piece of the puzzle of the climate evolution of Mars," Robert Lillis, principal investigator for ESCAPADE and associate director for planetary science at the University of California, Berkeley's Space Sciences Laboratory, said in a statement released Wednesday (Nov. 5). "ESCAPADE gives us what you might call a stereo perspective — two different vantage points simultaneously."
Geologic evidence from ancient river valleys and water-formed minerals shows that Mars once had liquid water, which means it also had a much thicker atmosphere. But around 4 billion years ago, the planet's magnetic field, which is the invisible shield that protects a world from the sun's radiation, began to fade. Without that protection, the solar wind slowly stripped away the Martian atmosphere, leaving behind a tenuous wisp less than 1% as dense as Earth's.
Previous missions, including NASA's Mars Global Surveyor, MAVEN, and the Emirates Mars Mission Hope, have shown that Mars lacks a global magnetic field but retains patchy magnetic "bubbles" locked into its crust. However, with only one spacecraft in orbit at a time, researchers have been limited to viewing one region at a time, often hours apart.
With the ESCAPADE satellites, "we can monitor how those regions vary on timescales as short as two minutes and up to 30 minutes," Lillis said in the statement. "This will allow us to really make measurements we've never made before, and to characterize a very dynamic system in a way we couldn't characterize it before."
After reaching Mars in September 2027, the robotic duo will spend about seven months fine-tuning their orbits before flying in formation, like a "pair of pearls on a string," coming within 100 miles (160 kilometers) above the surface. If all goes to plan, after six months of joint observations, they will separate into different orbits for another five months to build a 3D map of how energy and matter flow between Mars and the solar wind, the process that controls atmospheric loss.

Over roughly 11 months of science operations, ESCAPADE will explore three key questions, including how Mars’ magnetic bubble is shaped, how energy from the sun interacts with it, and how this affects the flow of particles in and out of the planet’s atmosphere.
To achieve this, each probe, about the size of a copy machine, carries an identical suite of instruments working in concert. Electrostatic analyzers, built at UC Berkeley, will detect charged particles escaping from Mars; by measuring their direction and energy, scientists can determine whether those particles are falling back toward the planet or being swept away by the solar wind, the statement says.
A magnetometer from NASA's Goddard Space Flight Center will track the strength and orientation of magnetic fields, while plasma sensors from Embry-Riddle Aeronautical University will probe plasma properties. Meanwhile, student-built cameras from Northern Arizona University will capture images of Mars, and may even catch glimpses of its mysterious green auroras.
ESCAPADE is also testing a clever new route to Mars. Instead of heading directly to Mars, the spacecraft will first gear toward a Lagrange point, a gravitational “sweet spot” between Earth and the sun, for about a year before slingshotting toward Mars in 2026. This longer but more flexible route could make future missions less dependent on the narrow, once-every-two-years Mars launch windows, scientists say.
Understanding how solar radiation interacts with Mars' upper atmosphere, known as the ionosphere, could also aid future explorers. On Mars, radio waves can reflect off the ionosphere to travel beyond the horizon, so mapping how this layer behaves will be vital for communication and navigation. The mission's results may even hint at whether liquid water still lingers underground, a possibility supported by recent analyses of seismic data from NASA's InSight lander — and a key question for future human exploration.
"It is definitely going to be a challenge to establish a human settlement on Mars," Lillis said in the same statement. "But, you know, humans are tenacious, right?"
Blue Origin's powerful New Glenn rocket will launch a NASA mission to Mars this weekend, and you can watch the action live.
The twin ESCAPADE Mars probes are scheduled to lift off atop the partially reusable New Glenn from Florida's Cape Canaveral Space Force Station on Sunday (Nov. 9), during a 2.5-hour window that opens at 2:45 p.m. EDT (1945 GMT).
You can watch the launch — the second-ever for New Glenn — live via Blue Origin, which was founded by Amazon's Jeff Bezos. Space.com will carry the feed as well, if the company makes it available.

ESCAPADE (short for "Escape and Plasma Acceleration and Dynamics Explorers") will be the first Mars mission to launch in more than five years, since NASA's Perseverance rover and Ingenuity helicopter lifted off together on July 30, 2020.
The $80 million ESCAPADE mission consists of two spacecraft, which were built by Rocket Lab and will be operated for NASA by the University of California, Berkeley. That latter fact explains the duo's names — Blue and Gold, which are UC-Berkeley's school colors.
New Glenn will launch Blue and Gold toward the Earth-sun Lagrange Point 2 (L2), a gravitationally stable spot about 930,000 miles (1.5 million kilometers) beyond our planet.
The pair will hang out there for 12 months while studying space weather. They'll loop by Earth in November 2026, getting a gravitational boost from our planet to head out to Mars, which they'll reach about 10 months later.
This complex trajectory is required by orbital dynamics: Earth and Mars align just once every 26 months for efficient interplanetary travel, and the next such window opens in late 2026.
After they reach the Red Planet, the ESCAPADE probes will spend about seven months lowering themselves into precisely aligned orbits, then gather data for at least 11 months.
The orbiters will "fly in formation to map the magnetic fields, upper atmosphere and ionosphere of Mars in 3D, providing the first stereo view of the Red Planet’s unique near-space environment," UC-Berkeley wrote in a mission description.
"What they find will help scientists understand how and when Mars lost its atmosphere and provide key information about conditions on the planet that could affect people who land or settle on Mars," the university added.
Sunday's launch will be the second to date for New Glenn, which can haul about 50 tons (45 metric tons) of payload to low Earth orbit.
The rocket debuted with a successful test flight on Jan. 16, 2025, which sent a prototype version of Blue Origin's Blue Ring spacecraft platform to orbit.
The company failed in its attempt to land New Glenn's first stage on a ship at sea that day. It will try this landmark maneuver again on Sunday, so there will be lots of action for space fans to watch.
]]>We've reached out across time and space to build this list, looking at modern hits and bona fide classics. Real-time strategy, turn-based, grand strategy, squad-based tactics — it's all on the table. The only rule here is that this is a list of boots-on-the-ground strategy games; after all, the troops do the dying, the fleet just does the flying. Check out our best space strategy games list if you want to command fleets of starships.
Looking for more great space and sci-fi games? We've also covered the best space exploration and settlement games for players who want to unwind a bit, but if you're feeling more adventurous, check out our favorite space flight sims and space horror games too.
Release date: April 26, 2022 | Platforms: PC, Xbox Series X|S | Developer: Shiro Games
We'd been wishing for new Dune video games for the longest time, but it took the success of Denis Villeneuve's two movies to usher in a new era of Arrakis-set games worth putting the stillsuit on.
We're big fans of Spice Wars, a criminally underrated strategy title that mixes 4X and real-time strategy elements in a familiar sandy setting. It's a killer pitch, and the moment-to-moment gameplay is unlike any other RTS in the market right now. Just be aware, this one isn't beginner-friendly at all.
While much of the governing aesthetic is (obviously) borrowed from the Legendary-produced movies, it was nice to see developer Shiro Games put its own stamp on the visuals and art, too. What's often been a muted and dull-ish universe in other hands really pops in Spice Wars; from the heroic units of House Atreides to the menacing hordes backed by the Harkonnen, there's a nice blend of familiar designs and fresh takes on Frank Herbert's material.
Release date: August 6, 2019 | Platforms: PC, macOS, PS4, Xbox One | Developer: Triumph Studios
Yes, we know, Age of Wonders has traditionally been a fantasy 4X game series, but 2019's entry finally took things into outer space.
The result? A wild turn-based strategy game that embraces unique factions and unit design while putting its own spin on tried-and-tested 4X strategy systems and mechanics you might be familiar with. Age of Wonders: Planetfall is one of the most approachable games in this list.
From dinosaur-riding Amazons to cyborg-zombies, Age of Wonders: Planetfall certainly leans on a "fun-first" mentality, but despite that, it's shockingly well-balanced. There's even a compelling narrative, as you "uncover the history of the fallen galactic empire" by exploring the world, conquering new regions, and dealing with other civilizations through peace or war.
It also supports online, local, and asynchronous multiplayer. On top of everything, it's got a thriving modding scene thanks to official tools.

Release date: November 13, 2001 | Platforms: PC, macOS | Developer: LucasArts, Ensemble Studios, Westlake Interactive
Star Wars: Galactic Battlegrounds already made our top 10 Star Wars video games list with its surefire 'reskin' of classical Age of Empires gameplay and lovely isometric 2D sprites, but it deserves a spot here too. You don't need to reinvent the wheel to have a lasting impact, and Galactic Battlegrounds is one of those sci-fi strategy games that always feel great to boot up for a game or two, alone or with friends.
Between the surprisingly well-rounded campaigns and infinitely replayable skirmish mode, RTS games don't get much better. It covers multiple eras across the Star Wars timeline, too, so you can mash Gungan armies and Imperial stormtroopers together and create the battles that Lucasfilm never would.
In an age when most new Star Wars games target fidelity and try not to break the canon, it's fun to go back to LucasArts' more offbeat projects and be reminded that some famous IPs could stand being more flexible.
Release date: February 27, 2018 | Platforms: PC, Linux, macOS, iOS, Android, Nintendo Switch | Developer: Subset Games
Another entry we've talked about before (this time on our best mech games list), Into the Breach more than earns its spot here, too. Developed by Subset Games (makers of the excellent FTL: Faster Than Light), Into The Breach is an overlooked banger that we can't get enough of.
Like in many other mech tales, the threat is an alien invasion, but this time these monsters come from below, not above. Don't be fooled by the charming pixel art style and adorably small-scale battlefields; this is one of the deepest and most addicting strategy games of the last decade.
Into the Breach embraces randomly-generated elements into each run to keep things interesting and challenging even after you figure out the pilots, enemies, and mechs. It's the ultimate 'lean and mean' turn-based strategy game.
And as a bonus for sci-fi nerds, the developers even brought in Chris Avellone (Star Wars: Knights of the Old Republic II) as a guest writer to help with its original story and world.

Release date: March 2, 2010 | Platforms: PC, macOS, Xbox 360 | Developer: Gas Powered Games, Virtual Programming
Supreme Commander 2 remains one of the undisputable gold standards of massive-scale RTS games. It may not be the deepest or tightest of the bunch, but its developers went all out with a unique take on the classics, embodying the adage "go big or go home" with reckless abandon.
Set in the 39th century on the planet Altair II, an assassination sparks a tinderbox that leads to an epic three-faction war across the planet, as former allies become bitter rivals. The UEF, Cybrans, and Illuminate all have their own unique playstyles, with strengths to leverage and weaknesses to exploit.
Battles in Supreme Commander 2 are next level. Mechs, land, sea, and air vehicles fill the screen as factories and other buildings expand to fuel the war machine. The action quickly ramps up, and then it just never stops.
Some players argue to this day that the first game was more complex, and they might be right, but Supreme Commander 2's quality-of-life changes and accessibility-oriented tweaks give it the edge in our mind.
Release date: March 26, 2007 | Platforms: PC, macOS, Xbox 360 | Developer: EA Los Angeles
Command & Conquer is arguably the most iconic RTS franchise of all time, and almost all of its entries could be classified as sci-fi. But which is the best of the bunch? An argument can be made for plenty of them (our Entertainment Editor thinks it's Red Alert 2), but this is my list, so I'm going with C&C3: Tiberium Wars.
It just feels like the perfect middle point between old-school real-time strategy and welcome modernisations, and we appreciate the effort to push the story forward in big ways. We even like the controversial Scrin extraterrestrial invaders, and kind of wish they had a bigger showing in the campaign missions, too. Speaking of which, RTS story campaigns don't get much better than Tiberium Wars' 38-mission offering, complete with the franchise's legendary live-action cutscenes.
Nowadays, Command & Conquer has been all but abandoned by publisher EA, but its legacy can't be ignored, and if you're curious about it all, the third mainline installment might be the perfect way to fall in love with the series.

Release date: February 9, 1999 | Platforms: PC, Linux, macOS | Developer: Firaxis Games
As a spiritual successor to the enduring Civilization series, Sid Meier's Alpha Centauri was maybe a bit too offbeat for franchise regulars, but it still carved out its own legacy by doing its own thing in a distinct sci-fi universe.
Alpha Centauri… sorry, Sid Meier's Alpha Centauri takes players to the 22nd century, when seven human factions land on the planet Chiron in the Alpha Centauri system. Once there, everyone works together and they're all best buds… nah, obviously the usual petty conflicts break out, leading to some classic 4X turn-based strategy action.
Anyone going into Alpha Centauri for the first time in 2025 should know its user interface and pacing feel rough by today's standards, but if you can get past those obstacles early on, you'll soon discover one of the most engrossing strategy games of all time.
Many have tried to recapture Alpha Centauri's magic – including Firaxis themselves, who took Civilization to space with Civilization: Beyond Earth – yet no one was able to fully replicate the original's charm. We'll be patiently waiting for a true heir to the throne, but in the meantime, we'll be repeatedly replaying this masterpiece.
Release date: September 20, 2004 | Platforms: PC | Developer: Relic Entertainment
Walk softly, and carry a big gun. We've been banging the 'Dawn of War is the best Warhammer 40K game of all time' drum for a while now, and we stand by it, but we're also comfortable saying it's among the best sci-fi strategy games ever, period.
Dawn of War has excellent story campaigns, extensive rosters of units across several of the most iconic factions in the WH40K universe, a neat 'army painter' tool to help you recreate your tabletop 40K forces in-game, and tons of skirmish maps to play offline and online.
Relic Entertainment was at its peak when it unleashed this one, and the expansion packs only made it more enticing (especially Dark Crusade). We also just received a solid remaster, which makes enjoying one of the finest RTS games around easier than ever.
With Dawn of War 4 coming in 2026 (if the Emperor allows) and aiming to honor the original, that Definitive Edition's timing is utterly perfect. Even if you only have a passing interest in Warhammer 40,000, make sure to check this one out.
Release date: February 5, 2016 | Platforms: PC, Linux, macOS, iOS, Android, PS4, Xbox One, Nintendo Switch | Developer: Firaxis Games
If you don't count Space Invaders, the rebooted XCOM games are undoubtedly the best alien invasion games of all time, and if we had to choose a favourite amongst them, we'd go with XCOM 2 any day of the week.
After Earth's unconditional surrender, the aliens rule the planet, yet some remain committed to fighting against the extra-terrestrial oppressors. It's a killer pitch, and the sequel delivered on all fronts.
With the remaining XCOM forces now on the run, an alien craft becomes a mobile HQ, and inverting the dynamic of the war (making humans the 'invaders' trying to disrupt an established system) made for pretty fun story and gameplay changes. Make sure you're prepared to deal with a crushingly hard turn-based game though. Each mistake could be your' last, and losing fully kitted soldiers to dumb mistakes stings hard.
Release date: July 27, 2010 | Platforms: PC, macOS | Developer: Blizzard Entertainment
What can we say after all this time? StarCraft 2 is the best real-time strategy game of all time, never mind just sci-fi entries, so of course it's grabbed the top spot here. And how did Starcraft achieve such dominance? By keeping things remarkably simple.
There are only three factions — the Terrans, Protoss, and Zerg — but each has its own distinct playstyle, units, and strategies. The core gameplay loop is intuitive and approachable, while still offering a sky-high skill ceiling for competitive players to duke it out, and the campaign narrative takes some universe-altering swings as the story is told through gameplay and stunning CGI cutscenes.
Some diehard fans still prefer the original Starcraft, and we respect that, but having replayed both recently, there's no contest for us. StarCraft 2 isn't just a graphical upgrade; it iterated on everything that made the first game special and then took everything to the next level. We may never get another RTS like it ever again.
]]>Enterprise is available as a hefty 3,600-piece set in version NCC-1701-D, which was used during Star Trek: The Next Generation (1987-94) as well as the Star Trek: Generations movie of 1994 — as well as many spinoffs. The vehicle will warp into stores and online on Nov. 28, and retails for $399.99. It's recommended for fans who are 18+, although we're sure many grownups will be glad to construct this Trek icon alongside the kids.
If you hit warp speed on this purchase and buy before Dec. 1, you'll get a bonus: a Type 15 Federation Lego shuttlepod — Onizuka, named as a tribute to the real-life NASA astronaut Ellison Onizuka who died aboard space shuttle Challenger in 1986 — is available as a gift with purchase of the whole set.
Lego and partner Paramount Products & Experiences are planning some Black Friday events to celebrate, although you'll have to source your own Romulan ale. Lego insiders can enter a sweepstakes until Dec. 1 to win a signed set from Jonathan Frakes, a Star Trek actor and director best known for playing Commander William Riker (also known as "Number 2"). And on Nov. 28 between 10 a.m. and 12 p.m. in London, Star Trek fans can meet designer Hans Burkhand Schlömer at the store in Leicester Square to get Schlömer's signature on their starship purchases.
"As Commander Riker, I spent a lot of time on the bridge of the Enterprise, and now fans can take the helm themselves in Lego brick form," Frakes said in a statement from Lego. "This set is a fantastic way to relive the adventures of the crew, piece by piece."
The interior of the Onizuka includes a display showing Stardate 45076.3, along with a schematic of a Romulan spacecraft. (TNG superfans will recognize the stardate from the Season 5 episode "Ensign Ro" in 1991, which is a nice Easter egg as the Bajornan ensign herself is a minifigure with the craft.)

The "highly detailed replica of Starfleet's legendary flagship", as Lego terms the set, comes with nine minifigures that comprise the main TNG crew and famous Enterprise members: Captain Jean-Luc Picard, Riker, Lieutenant Worf, Lieutenant Commander Data, Dr. Beverly Crusher, Lieutenant Commander Geordi La Forge, Counselor Deanna Troi, Bartender Guinan, and even Wesley Crusher (son of Beverly)—who was with TNG for about half its run.

The starship also includes "a detachable command saucer, secondary hull, warp nacelles with distinctive red and blue detailing, an opening shuttlebay, 2 mini shuttlepods and an angled display stand with a schematic and ship statistics," Lego stated. The set is sized for a bookshelf or a desk, with dimensions (including stand) of 10.5 inches (27 cm) high, 23.5 inches (60 cm) long and 18.5 inches (48 cm) wide.

Accessories include the inevitable tricorder, a teacup (in a nod to Picard's spare-time habits), a phaser (never leave the ship without one), as well as an engineering case, PADD, bottle, portable tractor beam generator and — for the Data fans — a cat figure.
Make sure to buy this set quickly to have some fun work to better yourself, as well as the rest of humanity who loves this series. It'll be sure to sell out quickly given TNG's enduring popularity among fans.
]]>If you got a nickel every time SpaceX launched another batch of its Starlink broadband satellites, you wouldn't be rich, but you'd have a lot of nickels.
Under such an arrangement, today (Nov. 6) would mark another payday, as SpaceX did, in fact, launch another Starlink mission this afternoon.
Starlink Group 11-14 lifted off atop a Falcon 9 rocket from Vandenberg Space Force Base in California today at 4:13 p.m. EST (2113 GMT; 1:13 p.m. local California time), carrying 28 satellites to join the company's growing megaconstellation in low Earth orbit (LEO).

It was the eighth flight for the first stage of this Falcon 9 booster, known as 1093, which completed a stage separation and successful deceleration burns, then aced a landing on a drone ship in the Pacific Ocean about 8.5 minutes after liftoff.
B1093 will now ride that ship, called "Of Course I Still Love You," back to port for refurbishment and future launches.
While B1093 made its way back to Earth, the Falcon 9's upper stage continued toward LEO, carrying the 28 Starlink satellites to their deployment point, where they are scheduled to be released about an hour into flight.
They'll join more than 8,800 other spacecraft in the Starlink megaconstellation, which provides wireless internet service to customers across the globe.
Today's launch was the 142nd Falcon 9 mission of the year, and the 102nd devoted to building out the Starlink network.
]]>3I/ATLAS is only the third object ever confirmed to have reached our solar system after originating in another planetary system, following 'Oumuamua in 2017 and 2I/Borisov in 2019. This time, space agencies around the world have been looking at any and all ways to study the invading comet, including repurposing spacecraft spread across the solar system.
The European Space Agency and NASA are known to have pointed their Mars spacecraft, including surface rovers, toward the comet when 3I/ATLAS, which is thought to be older than our solar system, passed by in early October. And now the China National Space Administration (CNSA) has revealed that its own Tianwen 1 spacecraft imaged the comet between Oct. 1 and Oct. 4, publishing images showing its path during this time, as well as a standalone photo from Oct. 3.

Tianwen 1 used its High-Resolution Imaging Camera (HiRIC) — somewhat comparable to HiRISE on NASA's Mars Reconnaissance Orbiter (MRO), but slightly lower resolution — to capture the comet moving against a stellar backdrop. The operation posed challenges, notably switching from imaging bright planetary surface features from low Mars orbit to tracking, from 18 million miles (28.96 million kilometers) away, a faint comet that's moving at 129,800 mph (58 km per second) and is just 3.5 miles (5.6 km) wide.
"Data acquired by a high-resolution camera was received, processed and displayed by a ground-based application system," according to CNSA's Nov. 5 statement. "The images clearly show the comet's distinctive features, consisting of a nucleus and a surrounding coma, with a diameter reaching several thousand kilometers."
CNSA says the comet imaging project was an important extension mission for Tianwen 1, stating that the ability to observe faint celestial bodies provided a chance to perform useful technical tests and accumulate experience for the second mission in China's deep-space exploration series, Tianwen 2, which launched in May and is on its way to sample a near-Earth asteroid.
Tianwen 1 is China's first planetary exploration mission. It launched in July 2020 and entered Mars orbit in February 2021. The mission's Zhurong rover successfully landed in Mars' Utopia Planitia region in May 2021 and operated on the surface for around one Earth year.
The amount of ice on the Arctic Ocean has depleted by more than 42% in response to rising temperatures since regular satellite monitoring began in 1979 — and the Arctic continues to warm faster than anywhere else on Earth, particularly due to human-driven global warming caused by things like burning coal for cheap power. In a few decades time we could see the Arctic Ocean free of ice all summer long. Besides the resultant rising sea levels as the ice melts, scientists want to learn more about how this change in sea ice affects the habitability of the Arctic and the wider world.
"If we can project the timing and spatial patterns of ice coverage decline in the future, it will help us understand warming, predict changes to food webs and fishing, and prepare for geopolitical shifts," said Frankie Pavia of the University of Washington in a statement.
Until now, it has been difficult to make accurate predictions about the Arctic sea ice in part because there have been no historical records to base predictions on. If we don't know how the sea ice responded to changes in climate in the past, we can't say for certain how it will respond in the future.
Which is where the cosmic dust comes in.
We are being gently doused in dust from space every day. If you place a bowl outside for a week, some of the dirt that gathers in it will be from space.
When the Arctic Ocean is covered in ice, the dust is prevented from reaching the sea floor. So when the ocean is largely absent of ice, more of the cosmic dust is able to settle as sediment.
Pavia led a team who went searching for this dust in sedimentary cores taken from three locations in the Arctic Ocean: one near the North Pole where there is ice present all year, one near the edge of the ice in September when ice coverage is at its annual lowest, and another at a site that was covered in ice in 1980, but no longer is.
In particular, Pavia's team was looking for sedimentary layers of the isotopes helium-3 and thorium-230. Each has a different origin. Helium-3 is present in cosmic dust, having been captured by dust grains from the sun's solar wind, whereas thorium is a decay product of naturally occurring uranium that has become dissolved in the ocean. At times of high ice abundance on the ocean, the ratio of thorium-230 to helium-3 should be higher than at times when there is less ice and more cosmic dust can reach the seabed.
"It's like looking for a needle in a haystack," said Pavia. "You've got this small amount of cosmic dust raining down everywhere, but you've also got Earth sediments accumulating pretty fast."
The cores provided a historical record chronicling periods when greater and smaller amounts of cosmic dust have reached the bottom of the ocean, corresponding to differing amounts of sea ice. The ice has waxed and waned over millennia, and the cores indicate that the dawn of the most recent ice age, beginning about 20,000 years ago, saw a decrease in the amount of cosmic dust on the seabed as ice covered the entirety of the Arctic all year round.
"During the last ice age there was almost no cosmic dust in the Arctic sediments," said Pavia.
When the ice began to melt and retreat as the ice age started to come to an end 15,000 years ago, the cores show that the amount of cosmic dust in the sediment on the sea floor began to increase.
What's most intriguing is what the cores tell us about what governs the amount of sea ice and how its presence, or lack thereof, can influence the balance of nutrients and hence the biosphere of the ocean.
The assumption had been that the loss of ice from the Arctic Ocean was governed by the temperature of the ocean, but the results from Pavia's group indicate that it has more to do with atmospheric temperatures instead. This is a crucial piece of information because the ocean takes longer to respond to climate change than the atmosphere. If true, then we may lose sea ice in the Arctic Ocean more quickly than we expected.
They also found that sea-ice coverage is correlated with how quickly nutrients in the ocean are consumed by biological processes. Tiny shells that were once worn by microbes called foraminifera were present in the cores, and a chemical analysis revealed how much of the total available nutrients they consumed when the microbes were alive at different points in the historical record. Pavia’s team found a correlation between increased consumption of nutrients and a lack of sea ice.
"As ice decreases in the future, we expect to see increased consumption of nutrients by phytoplankton in the Arctic, which has consequences for the food web," said Pavia. Long term, such productivity might not be maintained, causing delicate ecosystems both in the ocean and on the coast to collapse.
The results still leave some questions unanswered for now, such as why nutrient availability changes with the amount of sea ice present. One possible explanation is that with less ice, there is more room on the surface of the ocean for photosynthesizing algae that produce more nutrients. However, a competing effect would be the dilution of the nutrients by the melting sea ice, meaning there must be a delicate balance between the two processes.
The results were published on Nov. 6 in the journal Science.
]]>Get a subscription to Disney Plus, Hulu and ESPN Unlimited for just $29.99 a month.
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It's not all Disney Plus shows, of course; there's plenty of great sci-fi TV on Hulu too. The channel is home to Futurama, The Handmaid's Tale, Paradise, Rick and Morty, Legion, Firefly, and much more.
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The deal we've highlighted bundles Disney Plus, Hulu, and ESPN Unlimited with ads, but an ad-free version is also available for $38.99 per month (usual price $44.99).
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Check out our other guides to the best telescopes, binoculars, cameras, star projectors, drones, Lego and much more.
]]>A gibbous moon, like the one captured here, refers to a phase in which the moon is more than half illuminated but not yet full, or just after full, when it's starting to wane. This phase is important because it represents one of the moon's brightest periods, offering extended natural light at night.
For astronomers and stargazers, the gibbous phase provides excellent visibility for spotting lunar craters and highlands, while for ancient peoples and modern observers alike, it has long symbolized growth, transition and the fullness of cycles.
This photo was taken at Cerro Pachón, a mountain in Chile's Atacama Desert.

Thanks to the excess glow from the gibbous phase, moongazers can see dark splotches, or maria, across the surface of our moon. These maria were created when the moon had active volcanoes. Two very specific and important maria can be seen in this image: Mare Tranquillitatis (above left of center) and Mare Serenitatis (left of the moon's center). Both of these sites are part of humanity's rich legacy of visiting the moon.
You can learn more about moon landings and other features of the moon.
]]>A gibbous moon, like the one captured here, refers to a phase in which the moon is more than half illuminated but not yet full, or just after full, when it's starting to wane. This phase is important because it represents one of the moon's brightest periods, offering extended natural light at night.
For astronomers and stargazers, the gibbous phase provides excellent visibility for spotting lunar craters and highlands, while for ancient peoples and modern observers alike, it has long symbolized growth, transition and the fullness of cycles.
This photo was taken at Cerro Pachón, a mountain in Chile's Atacama Desert.

Thanks to the excess glow from the gibbous phase, moongazers can see dark splotches, or maria, across the surface of our moon. These maria were created when the moon had active volcanoes. Two very specific and important maria can be seen in this image: Mare Tranquillitatis (above left of center) and Mare Serenitatis (left of the moon's center). Both of these sites are part of humanity's rich legacy of visiting the moon.
You can learn more about moon landings and other features of the moon.
]]>The speedy CME is forecast to arrive late tonight or early Friday (Nov. 7) morning (UTC) and could trigger strong (G3) geomagnetic storm conditions, according to NOAA's Space Weather Prediction Center. This follows a surprise round of auroras overnight when a glancing CME arrival combined with lingering effects from a high-speed solar wind stream, and pushed geomagnetic activity to G3 levels, sparking auroras across the northern U.S., Canada and Europe.
NOAA and the U.K. Met Office both have G3 storm watches in effect for Nov. 6 and Nov. 7. If the incoming CME arrives as predicted and if the magnetic orientation is favorable for a good connection to Earth's magnetic field, it could supercharge auroras across high and possibly mid-latitude regions.
Space weather physicist Tamitha Skov described the current forecast as "an aurora photographer's dream starting now and lasting at least through the weekend," adding that G3 to G4 storm levels are possible by Friday as multiple CMEs interact with Earth's magnetic field.
A whole train of big #solarstorms are on their way, along with some smaller storms hitting now, and some fast solar wind! It is an #aurora photographers dream starting now and lasting at least through the weekend. Right now, the biggest of the storms should hit late Thursday or… pic.twitter.com/OL50yH72y7November 5, 2025

According to NOAA's Kp index forecast, geomagnetic storming is expected to last between Nov 6 and Nov. 7, with the highest activity predicted for tonight.
Based on the latest NOAA aurora forecast map, the following 22 U.S. States appear fully or partially above the aurora view line:
But remember, that auroras are highly unpredictable, so even if you're within the view line, you'll still need cloud-free skies, minimal light pollution, a clear view northward and a little bit of luck to catch the show.
If you're in one of the 22 U.S. states listed above, here are some tips for catching a glimpse of the display.
We recommend downloading a space weather app that provides aurora forecasts based on your location. One option I use is "My Aurora Forecast & Alerts," available for both iOS and Android. However, any similar app should work well. I also use the "Space Weather Live" app, which is available on iOS and Android, to get a deeper understanding of whether the current space weather conditions are favorable for aurora sightings.

Tonight's storm is being driven by a CME launched by an M7.4 solar flare on Nov. 5 from active region AR4274 — a large and magnetically complex sunspot that continues to rotate into better view of Earth. The CME is traveling at speeds of 1,100 to 1,400 km/s (around 2.5–3.1 million mph) and is expected to arrive late Nov. 6 or early Nov. 7 (UTC). It follows an earlier CME that likely triggered the overnight storm, which combined with lingering fast solar wind to temporarily push Earth's magnetic field to G3 conditions.
Solar wind is expected to remain elevated over the next couple of days due to a mix of CME activity and incoming coronal hole high-speed streams according to NOAA forecasters. The current G3 geomagnetic storm watch reflects a moderate to high level of confidence in timing, but the actual intensity will depend on the speed and magnetic field orientation of the CME when it reaches Earth.
Region AR4274 remains highly active and is still rotating to directly face Earth. Multiple significant flares have erupted from this region over the past 48 hours, some with associated CMEs still being analyzed. The U.K. Met Office warns that elevated geomagnetic activity could continue into the weekend and even into Nov. 9, especially if additional CMEs are launched in Earth's direction.
NOAA also notes that another flare from the same region (an M8.6) may have produced an additional CME, which could result in further storming depending on how it interacts with solar wind conditions.
If you're an aurora enthusiast, keep your camera batteries charged; the show may be far from over.
]]>Earlier today (Nov. 7), the anticipated arrival of a coronal mass ejection (CME) launched with the M7.4 flare on Nov. 5 was detected by spacecraft positioned at Lagrange Point 1 (L1), roughly 1 million miles (1.5 million kilometers) from Earth. "The leading edge of a CME, presumably from the M7.6 flare, reached L1 just before 5h UTC," aurora chaser Jure Atanackov wrote on X. "Solar wind speed increased to ~800 km/s, Bt increased to ~17 nT. Bz has been variable so far, reaching everything between +16 and -16 nT. If it manages to stabilize at strongly negative values for some time, then we will see a rapid increase in geomagnetic activity."
NOAA's Space Weather Prediction Center has a G3-G2 storm watch in place for Nov. 7 and Nov. 8 as Earth experiences continued impacts from multiple CMEs and a fast solar wind stream from a coronal hole.

According to NOAA's Kp index forecast, geomagnetic storming is expected to last between Nov 7 and Nov. 8.
Based on the latest NOAA aurora forecast map, the following 10 U.S. States appear fully or partially above the aurora view line:
But remember, that auroras are highly unpredictable, so even if you're within the view line, you'll still need cloud-free skies, minimal light pollution, a clear view northward and a little bit of luck to catch the show.
If you're in one of the 10 U.S. states listed above, here are some tips for catching a glimpse of the display.
We recommend downloading a space weather app that provides aurora forecasts based on your location. One option I use is "My Aurora Forecast & Alerts," available for both iOS and Android. However, any similar app should work well. I also use the "Space Weather Live" app, which is available on iOS and Android, to get a deeper understanding of whether the current space weather conditions are favorable for aurora sightings.

Tonight’s aurora display is being driven by the impact of a CME launched by an M7.4 solar flare on Nov. 5 from sunspot region AR4274 — a large, magnetically complex active region now rotating into better view of Earth. The CME, which had been traveling at speeds of 1,100 to 1,400 km/s (2.5–3.1 million mph), arrived at Earth early on Nov. 7 UTC, sharply increasing solar wind speed and magnetic field strength.
The current G3 (Strong) geomagnetic storm watch remains in effect as more solar material is expected to arrive through Nov. 8, including a second CME launched by an M8.6 flare later on Nov. 5. Meanwhile, fast solar wind from a nearby coronal hole continues to enhance the disturbance.
NOAA and the U.K. Met Office both forecast elevated activity to continue through Nov. 8–9, with the strongest geomagnetic conditions likely on Nov. 7, followed by moderate storming on Nov. 8 and gradually easing conditions on Nov. 9.
Region AR4274 remains highly active and continues to rotate to face Earth. Multiple significant flares have erupted from this region over the past 48 hours, some with associated CMEs still being analyzed. The U.K. Met Office warns that elevated geomagnetic activity could continue into the weekend and even into Nov. 9, especially if additional CMEs are launched in Earth's direction.
If you're an aurora enthusiast, keep your camera batteries charged; the show may be far from over.
Editor's note: This article was originally published on Nov. 6, 2025, and has since been updated on Nov. 7 at 5:30 a.m. EST (1030 GMT) to reflect NOAA and UK Met Office forecasts issued Nov. 7, including the confirmed CME impact and ongoing possible G3 storming. A quote from aurora chaser Jure Atanackov has also been added.
]]>
The overnight storm was likely triggered by a glancing CME arrival that combined with lingering effects from a high-speed solar wind stream, according to NOAA's Space Weather Prediction Center (SWPC). The result was a strong burst of auroral activity, with sightings reported across Europe, Canada and the northern U.S.
But more solar storms are still on the way, saving the biggest until last. The M7.4 solar flare that erupted on Nov. 5 also released a CME traveling between 1,100 and 1,400 km/s (around 2.5–3.1 million mph) and is expected to reach Earth later on Nov. 6 or early Nov. 7 (UTC), according to NOAA's SWPC. This incoming CME, combined with a fast solar wind stream from a nearby coronal hole, could trigger another round of strong geomagnetic storming over the next 24 to 48 hours.
A strong (G3) geomagnetic storm indicates that Earth's magnetic field is heavily disturbed by solar activity. These storms can cause intermittent satellite navigation issues and high-frequency radio disruptions, as well as voltage corrections in power systems, particularly at high latitudes.

Strong geomagnetic storms can also spark bright, dynamic auroras, sometimes much farther into mid-latitudes than normal. If you're located in Canada, northern Europe and the northern U.S., make sure you keep your eyes on the skies tonight, as we could be in for a treat.
Space weather physicist Tamitha Skov described the current forecast as "an aurora photographer's dream starting now and lasting at least through the weekend," adding that G3 to G4 storm levels are possible by Friday as multiple CMEs interact with Earth's magnetic field.
A whole train of big #solarstorms are on their way, along with some smaller storms hitting now, and some fast solar wind! It is an #aurora photographers dream starting now and lasting at least through the weekend. Right now, the biggest of the storms should hit late Thursday or… pic.twitter.com/OL50yH72y7November 5, 2025
Sunspot region AR4274 remains large and magnetically complex and is continuing to rotate to face Earth, which means more solar fireworks could follow in the coming days.
]]>
The overnight storm was likely triggered by a glancing CME arrival that combined with lingering effects from a high-speed solar wind stream, according to NOAA's Space Weather Prediction Center (SWPC). The result was a strong burst of auroral activity, with sightings reported across Canada and the northern U.S.
But more solar storms are still on the way, saving the biggest until last. The M7.4 solar flare that erupted on Nov. 5 also released a CME traveling between 1,100 and 1,400 km/s (around 2.5–3.1 million mph) and is expected to reach Earth later on Nov. 6 or early Nov. 7 (UTC), according to NOAA's SWPC. This incoming CME, combined with a fast solar wind stream from a nearby coronal hole, could trigger another round of strong geomagnetic storming over the next 24 to 48 hours.
A strong (G3) geomagnetic storm indicates that Earth's magnetic field is heavily disturbed by solar activity. These storms can cause intermittent satellite navigation issues and high-frequency radio disruptions, as well as voltage corrections in power systems, particularly at high latitudes.

Strong geomagnetic storms can also spark bright, dynamic auroras, sometimes much farther into mid-latitudes than normal. If you're located in Canada, northern Europe and the northern U.S., make sure you keep your eyes on the skies tonight, as we could be in for a treat.
Space weather physicist Tamitha Skov described the current forecast as "an aurora photographer's dream starting now and lasting at least through the weekend," adding that G3 to G4 storm levels are possible by Friday as multiple CMEs interact with Earth's magnetic field.
A whole train of big #solarstorms are on their way, along with some smaller storms hitting now, and some fast solar wind! It is an #aurora photographers dream starting now and lasting at least through the weekend. Right now, the biggest of the storms should hit late Thursday or… pic.twitter.com/OL50yH72y7November 5, 2025
Sunspot region AR4274 remains large and magnetically complex and is continuing to rotate to face Earth, which means more solar fireworks could follow in the coming days.
]]>United Launch Alliance (ULA) plans to launch the big and powerful ViaSat-3 F2 satellite to orbit tonight (Nov. 6) after a one-day delay, and you can watch the action live.
ViaSat-3 F2, which weighs about 13,000 pounds (5,900 kilograms), is scheduled to lift off atop an Atlas V rocket today from Florida's Cape Canaveral Space Force Station, during a 44-minute window that opens at 10:16 p.m. EST (0316 GMT on Nov. 7). The launch was originally planned for Wednesday night (Nov. 5), but ULA scrubbed that attempt due to an issue with the rocket.
You can watch the launch live here at Space.com courtesy of ULA, or directly via the company. Coverage will begin about 20 minutes before liftoff.

If all goes according to plan tonight, the Atlas V will deploy ViaSat-3 F2 into geostationary transfer orbit about 3.5 hours after liftoff. The satellite will then spend several months making its way to geostationary orbit (GEO), a circular path that lies 22,236 miles (35,786 kilometers) above Earth.
At this altitude, orbital speed matches our planet's rotational speed. Satellites in GEO therefore "hover" over the same patch of Earth continuously, making it a popular destination for spy and communications craft.
ViaSat-3 F2 is expected to start beaming broadband service to customers in early 2026. As its name suggests, it will be the second ViaSat-3 satellite to do so, after ViaSat-3 F1, which launched atop a SpaceX Falcon Heavy rocket in April 2023. A third such craft is expected to launch next year, rounding out the ViaSat-3 constellation.
Each ViaSat-3 satellite is "designed to be capable of rapidly shifting capacity throughout its coverage area to deliver bandwidth where and when it’s needed most," Viasat, a California-based telecom company, wrote in a description of the mini constellation.
"This is important to meet the increasing demand of commercial, consumer and defense customers, where the location of high-demand hotspots can change over the course of the day," the company added.
According to that description, ViaSat-3 F1 provides connectivity primarily to airline passengers. ViaSat-3 F2 will "add more than 1 Tbps capacity to our network over the Americas," and ViaSat-3 F3 will do the same for the Asia-Pacific region.

The Atlas V has flown more than 100 missions since its 2002 debut, but its days are numbered.
ULA plans to retire the workhorse rocket in 2030 or thereabouts and has already fielded a replacement — the Vulcan Centaur, which has three launches under its belt to date.
Editor's note: This story was updated at 11:15 p.m. EST on Nov. 5 with news of the new target launch date of Nov. 6.
]]>ViaSat-3 F2, which weighs about 13,000 pounds (5,900 kilograms), had been scheduled to lift off atop an Atlas V rocket Thursday night (Nov. 6) from Florida's Cape Canaveral Space Force Station. ULA scrubbed the try, however, citing an issue "with the Atlas V booster liquid oxygen tank vent valve."
The same issue also caused a scrub on Wednesday night (Nov. 5). ULA has not announced a new target date; it will do so after investigating the rocket further.

On launch day, whenever that may be, the Atlas V will deploy ViaSat-3 F2 into geostationary transfer orbit about 3.5 hours after liftoff. The satellite will then spend several months making its way to geostationary orbit (GEO), a circular path that lies 22,236 miles (35,786 kilometers) above Earth.
At this altitude, orbital speed matches our planet's rotational speed. Satellites in GEO therefore "hover" over the same patch of Earth continuously, making it a popular destination for spy and communications craft.
ViaSat-3 F2 is expected to start beaming broadband service to customers in early 2026. As its name suggests, it will be the second ViaSat-3 satellite to do so, after ViaSat-3 F1, which launched atop a SpaceX Falcon Heavy rocket in April 2023. A third such craft is expected to launch next year, rounding out the ViaSat-3 constellation.
Each ViaSat-3 satellite is "designed to be capable of rapidly shifting capacity throughout its coverage area to deliver bandwidth where and when it’s needed most," Viasat, a California-based telecom company, wrote in a description of the mini constellation.
"This is important to meet the increasing demand of commercial, consumer and defense customers, where the location of high-demand hotspots can change over the course of the day," the company added.
According to that description, ViaSat-3 F1 provides connectivity primarily to airline passengers. ViaSat-3 F2 will "add more than 1 Tbps capacity to our network over the Americas," and ViaSat-3 F3 will do the same for the Asia-Pacific region.
The Atlas V has flown more than 100 missions since its 2002 debut, but its days are numbered.
ULA plans to retire the workhorse rocket in 2030 or thereabouts and has already fielded a replacement — the Vulcan Centaur, which has three launches under its belt to date.
Editor's note: This story was updated at 11:15 p.m. EST on Nov. 5 with news of the new target launch date of Nov. 6. It was updated again at 10:10 p.m. T on Nov. 6 with news of that day's launch scrub.
]]>Three of the VLT's massive domes were recently treated to this view of the Milky Way. Above the observatory, a soft green and red glow, known as airglow, helps to tinge the horizon. Airglow is a natural phenomenon arising from chemical reactions high in Earth's upper atmosphere, where atoms and molecules release light in the process. Depending on which elements are involved, airglow can appear in subtle shades of green, red or orange.
The VLT is based in the Andes Mountains in the Atacama Desert.

Airglow is incredibly faint, and invisible in most parts of the world because of widespread light pollution. Only in some of Earth's darkest places, such as the Atacama Desert, can this natural radiance be seen. It is precisely these conditions that make the VLT's site one of the best observing locations on the planet.
Astronomers are increasingly concerned that even remote observatories like the VLT may one day face the creeping glow of artificial light. Urban expansion, satellite constellations and industrial development all threaten to erode the natural darkness that makes sites like the Atacama Desert invaluable. Protecting these rare darkness sanctuaries is not only an environmental issue, but a scientific and culture one.
You can learn more about the Very Large Telescope and ground-based telescopes.
]]>Three of the VLT's massive domes were recently treated to this view of the Milky Way. Above the observatory, a soft green and red glow, known as airglow, helps to tinge the horizon. Airglow is a natural phenomenon arising from chemical reactions high in Earth's upper atmosphere, where atoms and molecules release light in the process. Depending on which elements are involved, airglow can appear in subtle shades of green, red or orange.
The VLT is based in the Andes Mountains in the Atacama Desert.

Airglow is incredibly faint, and invisible in most parts of the world because of widespread light pollution. Only in some of Earth's darkest places, such as the Atacama Desert, can this natural radiance be seen. It is precisely these conditions that make the VLT's site one of the best observing locations on the planet.
Astronomers are increasingly concerned that even remote observatories like the VLT may one day face the creeping glow of artificial light. Urban expansion, satellite constellations and industrial development all threaten to erode the natural darkness that makes sites like the Atacama Desert invaluable. Protecting these rare darkness sanctuaries is not only an environmental issue, but a scientific and culture one.
You can learn more about the Very Large Telescope and ground-based telescopes.
]]>President Donald Trump just tapped the billionaire tech entrepreneur to lead the U.S. space agency, five months after pulling his nomination for the same post.
"Jared's passion for Space, astronaut experience, and dedication to pushing the boundaries of exploration, unlocking the mysteries of the universe, and unlocking the new Space economy, make him ideally suited to lead NASA into a bold new Era," Trump wrote Tuesday (Nov. 4) in a post on Truth Social, the social media platform he owns.

That astronaut experience is extensive. Jared Isaacman, who founded the payments company Shift4, has organized, funded and commanded two private astronaut missions to Earth orbit, both of them using SpaceX hardware. On the second of those flights, called Polaris Dawn, he conducted the first-ever private spacewalk.
This will be Isaacman's second trip down nomination lane. Trump put him up for NASA chief this past January, and Isaacman looked set to be confirmed by Congress — until the president abruptly pulled his nomination on May 31, citing Isaacman's past donations to Democratic political candidates and supposedly close relationship with SpaceX founder and CEO Elon Musk.
Isaacman apparently isn't holding a grudge; he said he's ready to go through the process all over again.
"Thank you, Mr. President @POTUS, for this opportunity. It will be an honor to serve my country under your leadership," Isaacman said in a post on X, the social media platform that Musk owns, on Tuesday evening.
"The support from the space-loving community has been overwhelming. I am not sure how I earned the trust of so many, but I will do everything I can to live up to those expectations," he added.
NASA is currently led, in an acting capacity, by Sean Duffy, the former timber-sports champion and reality TV star who also serves as the Secretary of Transportation.
Duffy had been angling to hold on to the NASA job, according to media reports. But he struck a conciliatory and congratulatory tone in his own X post on Tuesday.
"Thank you @realDonaldTrump for the honor to lead @NASA. We’ve made giant leaps in our mission to return to the moon before China. It’s critical for our national security and national pride that we win the next space race. Congratulations to @rookisaacman. I wish him all the success and will ensure the transition is seamless," Duffy wrote.
Isaacman seems to enjoy widespread support from the space community, but his ascension to NASA chief is not a fait accompli — he still has to go through the confirmation process, which didn't end well last time. That confirmation process will likely be on hold due to the ongoing government shutdown, which has been underway since Oct. 1.
]]>This black hole is part of a collection of objects the James Webb Space Telescope (JWST) has been discovering in the early cosmos called "little red dots," mysterious specks of light that were only recently discovered thanks to the incredibly powerful infrared eye of this $10 billion space telescope. However, with a mass equivalent to 100 million times that of the sun, there is really nothing "little" about this black hole at all, with the discovery team dubbing it "BiRD," which stands for Big Red Dot.
Black holes don't emit any light themselves, in fact trapping any incident light due to their immense gravitational influence, but when these cosmic titans are surrounded by a wealth of matter upon which they are feeding, this material and jets blasted out from the poles of the black holes create a very conspicuous and bright object called a quasar. These can be seen from vast distances; for example, the light from BiRD has been travelling to Earth for 10 billion years.
BiRD was spotted in the region of the sky around a previously known quasar called J1030+0524 (J1030), itself a feeding supermassive black hole located around 12.5 billion light-years from Earth. This region of the sky has been well studied by astronomers — including this team, which hails from the National Institute for Astrophysics (INAF). However, it was while carefully analyzing images and spectra obtained with the JWST's Near-Infrared Camera (NIRCam) instrument that the research team detected an unusual source of light. A bright point in infrared that had never been revealed by prior X-ray and data.
"Starting from the calibrated images, a catalog of the sources present in the field was developed. It was there that we noticed BiRD: a bright, point-like object, which, however, was not a star and did not appear in the existing X-ray and radio catalogs," Federica Loiacono, team leader and INAF research fellow, said in a statement translated from Italian. "I analyzed its spectrum, which tells us about the chemical composition and some of the physical properties of the object."
This is possible because elements absorb and emit light at specific and characteristic frequencies. This means that the elements leave their "fingerprints" in wavelengths of light, or spectra.
"We found clear signals of hydrogen — in particular the line called Paschen gamma, a luminous signature that reveals the presence of ionized hydrogen — and helium, also visible in absorption," Loiacono said. "These details allowed us to estimate the distance to BiRD, discovering that it is relatively close to us compared to most of the little red dots known to date. Also from the analysis of the spectrum of this source, we were able to estimate the mass of the central black hole: about 100 million times that of the sun."
Little red dots are very compact objects with curious spectroscopic characteristics. Many possible theories exist surrounding these bodies, including a recent suggestion that they could be a new class of celestial body called "black hole stars." One of the prevailing theories posits that little red dots are feeding and growing supermassive black holes. The problem with this concept is the fact that the region around ravenous black holes should emit strongly in the X-ray region of the electromagnetic spectrum, but that doesn't seem to be the case for little red dots or for BiRD.
One possible explanation for this is that little red dots are the massive black hole "seeds" from which supermassive black holes grow and are therefore still shrouded by thick shells of gas and dust, shrouds that absorb high-energy X-ray radiation while allowing low-energy infrared light to slip through.
But even among the known little red dots, BiRD is a strange example.
"Before BiRD, only two other little red dots with the same spectral characteristics, including helium lines and Paschen gamma rays, were known at this same cosmic distance," Loiacono explained. "Comparing the spectral properties of BiRD with those of the other two, we found strong similarities: the line widths, absorption, black hole mass, and gas density are very similar. This led us to conclude that BiRD belongs to the same family as little red dots."
In addition to the discovery of BiRD, this research could change how scientists think of little red dots and, in turn, the growth and evolution of supermassive black holes. It was previously thought that these objects would have started to disappear as cosmic noon rolled around approximately 11 billion years ago. However, this team performed a calculation estimating the abundance of little red dots during cosmic noon, finding them to still be numerous during this cosmic epoch.
"The challenge now is to extend the study to a larger number of nearby LRDs, which we can study in greater detail than distant ones, to build a more complete picture," Loiacono concluded. "JWST has opened a new frontier in extragalactic astrophysics, revealing objects we didn't even suspect existed, and we're only at the beginning of this adventure."
The team's research was published on Thursday (Oct. 30) in the journal Astronomy & Astrophysics.
Two bright meteors were caught slamming into the moon on Thursday (Oct. 30) and Saturday (Nov. 1), by Japanese astronomer Daichi Fujii, curator of the Hiratsuka City Museum. The flashes, visible from Earth for just a split second, were caused by space rocks striking the lunar surface at high speed, producing brief but brilliant explosions of light.
As the Southern Taurid meteor shower approaches its peak around Nov. 5 and the Northern Taurids follow on Nov. 9, meteors are already lighting up Earth's skies — and apparently that of the moon as well. Fujii recorded the impacts using cameras aimed at the moon's nightside, sharing the dramatic videos on his X account.
The first collision occurred at 8:30 p.m. Japan Standard Time (6:30 a.m. EST or 1130 GMT) on Oct. 30, while the second happened at 8:49 p.m. Japan Standard Time (6:49 a.m. EDT or 1149 GMT) on Nov. 1.
According to Fujii, the Oct. 30 flash appeared east of the Gassendi Crater. Based on his calculations, the impactor was likely part of the Taurid meteor stream, striking the moon at a velocity of 27 km/s (60,000 mph) and an angle of 35 degrees. The meteoroid's estimated mass was 0.4 pounds (0.2 kilograms), excavating a crater about 10 feet (3 meters) wide and producing a flash lasting just 0.1 seconds.
"The pixels were saturated, so it's possible the flash was even brighter than the recorded data suggests", Fujii told Space.com.
The second flash, on Nov.1, appeared west of Oceanus Procellarum, one of the moon's largest lunar maria.
While it's not yet confirmed whether these impacts originated from the Taurids or were simply sporadic meteors, Fujii notes the timing aligns with the showers' period of increased activity. This marks the latest in a series of lunar impact observations by Fujii, who has become one of the leading recorders of such events.

"I started observing lunar impact flashes around 2011 and have been continuously observing since 2020," Fujii said. "With my 20cm telescope, I typically detect about one impact flash every few dozen hours of observation. Because the thin crescent moon is visible only briefly and often low in the sky where thin clouds are common, I only observe a few dozen flashes per year".
Fujii has documented a total of 60 flashes so far.
Unlike Earth, which is shielded by a thick atmosphere that vaporizes most meteors before they reach the ground, the moon's virtually non-existent atmosphere means there is nothing to slow down incoming meteors, sending them crashing into its surface at speeds of 45,000 to 160,000 mph (20 to 72 km/s) — releasing powerful bursts of light and heat on impact.
Such impacts can excavate craters tens of feet across, even from meteoroids weighing just a few pounds. For example, a rock just 11 pounds (5 kilograms) in mass can gouge a crater more than 30 feet (9 meters) wide and eject over 75 metric tons of lunar soil and rock, according to NASA.
]]>The finding, based on data from the Daniel K. Inouye Solar Telescope in Hawaii, marks the first direct evidence of tiny twisting magnetic motions of energy-packed plasma waves in the sun's outer atmosphere, or corona, known as torsional Alfvén waves.
First predicted by Swedish Nobel laureate Hannes Alfvén in 1942, Alfvén waves are magnetic disturbances that travel through the plasma, the superheated, electrically charged gas that makes up the sun. Larger versions of these waves have been seen before, typically linked to solar flares, but the smaller, ever-present twisting kind had remained elusive — until now.
"This discovery ends a protracted search for these waves that has its origins in the 1940s," Richard Morton, a professor of engineering, physics and mathematics at Northumbria University in the U.K. who led the study, said in a statement.
Scientists have long suspected that these small-scale waves could continuously carry energy from the sun's surface into its atmosphere, powering the solar wind and heating the corona to millions of degrees, far hotter than the sun's visible surface, which is only about 9,932 degrees Fahrenheit (5,500 degrees Celsius).
The results offer crucial confirmation for theoretical models about how magnetic turbulence carries and dissipates energy in the sun's upper atmosphere, Morton added. "Having direct observations finally allows us to test these models against reality."
To arrive at their conclusions, Morton's team used data from the Inouye Telescope, which captures the highest-resolution images of the sun ever obtained. The four-meter-wide telescope can detect faint shifts in light that reveal how plasma moves through the corona, allowing scientists to see the sun in unprecedented detail.
During the telescope's commissioning phase in October 2023, the team tracked iron atoms heated to 1.6 million degrees Celsius and spotted faint red and blue shifts on opposite sides of magnetic loops, which were the telltale signature of twisting Alfvén waves, according to the study.
These waves twist the sun's magnetic field lines like a corkscrew, but the motion is too subtle to spot directly in images, scientists say. To detect them, Morton's team used spectroscopy, a technique that measures how hot gas moves toward or away from Earth. This motion slightly changes the light's color, red when moving away, blue when moving closer, thereby revealing the hidden twisting pattern in the sun's atmosphere.

"The movement of plasma in the sun's corona is dominated by swaying motions," Morton said in the statement. "These mask the torsional motions, so I had to develop a way of removing the swaying to find the twisting."
The results show that even in the sun's calmest regions, the corona is riddled with torsional Alfvén waves. These torsional Alfvén waves constantly turn the sun's magnetic field lines back and forth, carrying energy upward through its layers. These waves transport energy from the lower atmosphere into the corona, where it's released as heat, offering new insight into why the sun's outer atmosphere is millions of degrees hotter than its surface.
For Morton and his colleagues, the long-sought detection opens new potential investigations into how these waves propagate and dissipate energy in the corona.
A paper about these results was published on Oct. 24 in the journal Nature Astronomy.
They may not have all the fixins, but the astronauts aboard China's Tiangong space station are sure eating well.
A new oven delivered to Tiangong has been put to quick work by the six people currently living aboard the outpost, the astronauts of the Shenzhou 20 and Shenzhou 21 missions.
In a video released by the Astronaut Center of China (ACC), the space station crew is seen securing a set of chicken wings in a specially made grill cage and placing it in a small, cabinet-like compartment in the space station's wall.

The oven not only serves as a powerful technology demonstration for the microgravity microwave (which actually functions more like an air fryer), but it also provides a welcome flavor of home for the astronauts living aboard the station.
Kang Guohua, a senior member of the Chinese Society of Astronautics and a professor of aerospace engineering at Nanjing University of Aeronautics and Astronautics, told Chinese state media that comforts such as hot meals are important to keep crews psychologically "grounded."
According to the ACC, the oven operates without stressing Tiangong's power grid and is designed to provide consistent and smokeless baking conditions in the station's microgravity environment. Such conditions are necessary aboard orbital outposts like Tiangong and the International Space Station (ISS), which rely on strictly maintained life support systems and rigorous fire safety protocols.
Cooking in microgravity differs from cooking something here on Earth. The sweet spot for the chicken wings was 28 minutes inside their enclosed grill container. Some peppered steak was also prepared for Shenzhou 20 Commander Chen Dong, according to a report from the Global Times, a tabloid owned by the state-run People's Daily.
The Global Times compared the cooking milestone to one notched aboard the ISS in 2019, when NASA astronauts baked cookies in space using a prototype Zero G oven. That test showed that baking things in orbit (at least cookies) takes longer than it does on Earth. But China's oven, unlike the temporary Zero G oven used aboard the ISS, is there to stay. The device has been integrated into Tiangong's systems and certified for up to 500 uses.
The Shenzhou 21 crew launched to Tiangong on Oct. 31 and will remain aboard Tiangong for roughly six months. The trio is relieving the Shenzhou 20 astronauts, who have been living aboard the station since April and will return to Earth on Nov. 5.
]]>It's long been known that "everyday matter" is made up of atoms, which are, in turn, composed of protons, neutrons and electrons. We also know that these particles fall in line with the known fundamental forces of nature: electromagnetism, gravity, the strong nuclear force and the weak nuclear force. However, what has been less clear is whether dark matter obeys these same four forces. Indeed, one of the reasons dark matter is so puzzling is that it doesn't seem to act in conjunction with light, or electromagnetic radiation. And if it does, it does so much more weakly than ordinary matter does. This makes dark matter effectively invisible, meaning the only way scientists can infer its presence is by observing its gravitational effects and then watching how that acts as a middleman and impacts light and ordinary matter.
But determining that dark matter interacts gravitationally on relatively small scales, such as within galaxies, doesn't tell us if it obeys the well-understood laws of gravity as defined by Albert Einstein's 1915 theory of gravity, general relativity, on much larger cosmological scales. That is a big question because accounting for five times more of the matter in the universe than everyday matter, dark matter should have played a major role in how the cosmos developed.
To solve this conundrum and to discover if dark matter could be governed by a fifth, thus far unknown fundamental force, researchers from the University of Geneva (UNIGE) set about determining if dark matter falls into cosmic gravity wells on vast scales just as ordinary matter does. These gravity wells are created when bodies of tremendous mass cause the very fabric of space and time, unified as a single four-dimensional entity called "spacetime," to warp (as established by general relativity). The greater the mass of the body, the more extreme the warping of spacetime, the "deeper" the resultant gravity well, and thus the stronger the gravitational influence.
"To answer this question, we compared the velocities of galaxies across the universe with the depth of gravitational wells," Camille Bonvin, team member and UNIGE researcher, said in a statement. "If dark matter is not subject to a fifth force, then galaxies — which are mostly made of dark matter — will fall into these wells like ordinary matter, governed only by gravity.
"On the other hand, if a fifth force acts on dark matter, it will influence the motion of galaxies, which would then fall into the wells differently. By comparing the depth of the wells with the galaxies' velocities, we can therefore test for the presence of such a force."
With this approach and using up-to-date cosmological data, the team established that dark matter does indeed slip into gravity wells just as ordinary matter does. While these findings provide no hints of a fifth fundamental force of nature, they can't absolutely rule it out.
"At this stage, however, these conclusions do not yet rule out the presence of an unknown force. But if such a fifth force exists, it cannot exceed 7% of the strength of gravity — otherwise it would already have appeared in our analyses," Nastassia Grimm, team leader and researcher at the Institute of Cosmology and Gravitation, University of Portsmouth in the UK.
While these results don't close the book on a fifth force of nature governing dark matter, they do help better define the characteristics of this disturbingly elusive form of matter. And if there is a fifth force of nature, it likely won't be able to hide forever.
"Upcoming data from the newest experiments, such as LSST [the Legacy Survey of Space and Time conducted by the Vera C. Rubin Observatory and DESI [the Dark Energy Spectroscopic Instrument], will be sensitive to forces as weak as 2% of gravity," Isaac Tutusaus, team member and researcher at the University of Toulouse, said. "They should therefore allow us to learn even more about the behaviour of dark matter."
The team's research was published on Monday (Nov. 3) in the journal Nature Communications.
Seen as the runt of his clan, Dek has something to prove. He wants to assert himself as a top hunter and be accepted by his father, who is also his chief. As Schuster-Koloamatangi said in a press Q&A, hunting is how the Yautja gain status, much like how humans acquire money on Earth.
The following contains spoilers for "Predator: Badlands."

Dek's older brother Kwei (Mike Homik) harbors a quiet belief in Dek, but he knows the odds are firmly stacked against him. Especially after Dek chooses the planet Genna as his hunting ground and eyes the Kalisk as his prize.
Genna is widely recognized as one of the most dangerous planets in the entire galaxy, with everything in sight (including the unassuming plants and cute-as-a-button creatures) being potential threats. Then, there's the Kalisk – an apex predator that's apparently unkillable. According to Kwei, even their father fears the creature.
Before Dek's hunt even begins, he gets dealt a confidence-shaking blow: His father reveals that he ordered Kwei to kill him because he has no faith in him succeeding as a hunter. He's seen as a weakling, and he must be culled from the clan. Father offers Kwei a second chance to finish the assignment, but Kwei chooses to save his brother instead.

For his loyalty to his sibling, Kwei receives the unwelcome reward of being massacred in front of a helpless Dek. Kwei uses his last breath to send his brother to Genna, offering him a chance to at least attempt his first hunt.
Carrying a chip on his shoulder and anger in his heart about what happened to Kwei because of him, Dek barely survives his arrival in Genna. Reluctantly, he accepts the assistance of the creature Bud and damaged Weyland-Yutani synthetic Thia (Elle Fanning). Dek finds the Kalisk, but the rest of Weyland-Yutani's synthetics – led by Tessa (also Elle Fanning) – swoop in, gathering the Kalisk for themselves and capturing Dek in the process. Thanks to Thia's help, the Yautja escapes the corporation's clutches, but he finds himself trapped on Genna with no tech and no hope.

It's at this moment that the audience swears they hear the faint music from "The Lion King" when Mufasa appears to Simba in the clouds and urges him to remember who he is. Instead of Mufasa's voice, though, it's Thia's that Dek hears, encouraging him to be the lone wolf.
This is the turning point of "Predator: Badlands," as Dek accepts the cold, hard facts here. He isn't like the other Yautja; he's unique, and that makes him special in his own way. For too long, he sought to conform and be what they wanted him to be, in an attempt to gain their approval and entry into the Predator clubhouse. Yet, Kwei was the only one of his pack who offered him encouragement, and now he's gone, and so are Dek's chances of acceptance here. Dek is a Yautja outcast, but this doesn't mean he's alone in life. It's a classic tale of accepting yourself and not conforming to what society expects of you. It's Good Will Hunting, but with a lot more real hunting.
In Thia and Bud, Dek forms his own clan, proving that you can't choose the family you're born into, but you can choose the family you live with. While Dek's father and clan members refused to help Dek with his rite of passage, Dek's "new" family offered help from the get-go, expecting nothing of him in return.

What Thia and Bud receive is Dek's undying loyalty. When the chips are down, Dek comes back for them, proving the killer instinct has always resided in him, and he didn't need fancy tech or Yautja's stamp of approval to unleash the warrior within. The spirit isn't found in a hunt; it's either in you or it's not. In the past, Dek craved a sense of belonging and desperately wanted to fit in with the Yautja, but he's now found his purpose – his people – in an unexpected foreign planet. He channels all of his ferociousness and violence to fight for them – not trophy – and discovers who he is and where he belongs.
Dek doesn't succeed in claiming the Kalisk as a trophy – nor does he want to, as he gains respect for the creature that's eventually destroyed by Tessa – but he returns to his home planet to confront his father. It's a brutal homecoming, as Dek rejects his clan and claims revenge for what his father did to Kwei, but it is a cathartic moment for him and the audience. Dek is now free to fulfil his own destiny.
If "Predator: Badlands" sounds like a strange story for a Predator, that's because it is. Traditionally, the species is portrayed as a villain in the series as it hunts down and skins humans for sport and prestige. Now, here's Dek making friends with a synthetic and an intergalactic creature, cracking jokes about "tools," and rejecting his Yautja clan.

Here's the catch, though: Dek could still be the Predator who'll skin a person alive and use their intestines as a necklace, but there isn't a single human being present in this specific story to find out. It's all flora, fauna, and synthetic. By doing this, Trachtenberg showcases how it's possible to explore the duality of the Yautja without damaging the essence of the franchise by switching the character's relationship with humankind. He also avoids having to rerun the "Predator gains respect for the human" arc from Alien vs. Predator. Dek isn't above murder – not at all – so who knows how he would react if he encountered a human who rubs him up the wrong way?
No one sees themself as the villain of their own story, so it's unlikely the Yautja view their actions as evil in the other Predator movies either. What Trachtenberg does well in "Predator: Badlands" is to show how the Yautja and humans aren't so different after all, as everyone craves acceptance and belonging, but might be looking in the wrong place for it. Incredibly, the filmmaker succeeds in telling a deeply human story without a single human in sight, affirming that humanity – despite its name – isn't only a human trait.
Maybe audiences will look differently at Dek and the Yautja from now on, seeing them as more than intergalactic big game hunters… or it'll annoy just the purists who believe "Predator" should always be about the monstrous creature hunting down macho men in the forest and everyone trying to get to the chopper. For our part, we're glad to see a deeper answer to Dutch's question, "What the hell are you?"
"Predator: Badlands" hits theaters worldwide on November 7. The rest of the Predator movies, including Dan Trachtenberg's "Prey", can be found on Hulu (US) or Disney+ (UK).

Watch the Predator franchise, including Predator: Badlands, when it launches on Hulu in the US after its theatrical run.
You can find the available plans below:
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If you're living in the UK like me, or anywhere else outside the US, then you won't have access to Hulu. Fortunately, you'll find all the current Predator movies on Disney+.
Prices vary by country, but you can find the UK prices below for reference:
Standard (with ads): £5.99/month
Standard (no ads): £9.99/month or £99.90/year
Premium (4K): £14.99/month or £149.90/yearView Deal
The Japanese Aerospace Exploration Agency's Akatsuki mission orbiting Venus was declared dead last week after engineers spent more than a year trying to get in touch with the silent spacecraft. Akatsuki spent a decade orbiting the planet and was well beyond its design lifetime when its mission ended, giving unprecedented looks at the hellish atmosphere of Venus.
While this Venus mission is gone, more are on the books. But some of them are hanging by a thread, as they depend on NASA support at a time when the agency is facing unprecedented budget cuts. The Trump administration proposed a 24% reduction to the agency's fiscal 2026 budget, from $24.8 billion to $18.8 billion. While the U.S. House of Representatives and Senate have proposed more money for NASA, the U.S. budget is still in limbo as the government enters its second month of shutdown after the fiscal year began on Oct. 1.
Here is a list of proposed missions to Venus.
The $500 million DAVINCI mission is slated to launch in the early 2030s as a combination orbiter and descent probe. The orbiter will look at the clouds of Venus, as well as the planet's mountains, during two flybys. The 3-foot-wide (1 meter) descent probe will fall to the surface of Venus and catalog its punishingly thick atmosphere and sulfuric acid-laden clouds along the way, as well as take some images of Venus' surface terrain.
NASA says the spacecraft together will achieve several firsts, including looking for traces of any ancient water cycle on Venus. The mission will focus on Alpha Regio, a "tessera" highland region that has only been imaged through orbital radar instruments. These types of terrain may be billions of years old, making the region one of the oldest surfaces on Venus.
DAVINCI will also be the first mission to chart the chemical composition of the lower atmosphere of Venus, between 17 miles (27.5 kilometers) and the surface, which will allow scientists to learn more about how gases and chemical compounds work on the surface — and perhaps even the subsurface — of Venus. But that's assuming the spacecraft goes forward, as it is on the list of canceled missions in the Trump administration's 2026 NASA budget.
VERITAS will launch no earlier than 2031 to learn more about how Venus and Earth, which are roughly the same size, diverged so greatly in their planetary histories. Aims of the science include learning how the oceans and magnetic field of Venus disappeared, and how plate tectonics changed the terrain. Like DAVINCI, however, VERITAS will be canceled if Trump's 2026 NASA budget is enacted.
VERITAS, a half-billion-dollar mission, is based on the design of NASA's MAVEN (Mars Atmosphere and Volatile Evolution) spacecraft that has been orbiting Mars since 2014. The spacecraft is supposed to orbit around the poles of Venus to allow for views of the entire planet below. Initially the orbit will be 120 hours and highly elliptical, but managers plan a second burn of the engines that will allow VERITAS to circle the planet in only 10 hours.
VERITAS will then use a technique called "aerobraking," using the drag of the upper atmosphere of Venus to lower its orbit by reducing the speed of the spacecraft. This is a lengthy procedure, expected to last several months, but will allow the spacecraft to carry less fuel to Venus and prioritize that mass instead for instrumentation. Once that is finished, VERITAS will be able to go around the planet in 1.6 hours, for a mission expected to last for 2.5 Earth years.

Envision is slated to lift off no earlier than November 2031 aboard an Arianespace Ariane 6 rocket. Led by the European Space Agency (ESA), the mission will include a synthetic aperture radar from NASA as well as support from the American agency's Deep Space Network, which is a group of three large radio dishes that communicate with spacecraft across the solar system. NASA's contribution, however, is under threat following proposed cuts to its fiscal 2026 budget, ESA officials confirmed to Nature earlier this year.
The €610 million ($705 million) mission will cruise to Venus for 15 months, then aerobrake in the atmosphere for 11 months before reaching its science orbit, which will circle the planet in roughly 90 minutes. ESA says the mission will focus on the origins of habitability in the solar system, as Venus may have had a climate similar to that of Earth for billions of years before something triggered its oven-like conditions at the surface. The mission aims to spend four Earth years examining Venus from its subsurface to its upper atmosphere, including learning more about the planet's history while charting its current climate and activity.
The spacecraft will be an orbiter with several instruments: an S-band radar/microwave radiometer and altimeter that will map the surface of the planet; three optical spectrometers aiming to examine trace gases (including volcanic gases) as well as the composition of the surface; a subsurface radar sounder to examine the subsurface as far as 0.6 miles (1 km) below the surface; and a radio science experiment to look at Venus' gravity field, as well as atmospheric composition and structure.
Billed as the first private mission to explore Venus, Rocket Lab is partnering with the Massachusetts Institute of Technology (MIT) to launch a small spacecraft to Venus in search of the building blocks of life, organic compounds, in the cloud layers of Venus. The Venus Life Finder mission is expected to use Rocket Lab's Electron rocket and Photon spacecraft, which will orbit the planet roughly 30 miles (48 km) above the surface. It was originally slated to fly in early 2025, but after a delay the spacecraft may lift off in summer 2026.
The mission (pegged at just $10 million in media reports) includes a probe that is expected to fall into the atmosphere of Venus, taking data primarily at altitudes between 37 and 28 miles (60 to 45 kilometers). This region was chosen because there have been suggestions of phosphine there, and temperatures and pressures in this altitude range are similar to those on Earth.
During a science collection phase lasting only between three and five minutes, according to the Planetary Society, the mission's laser science instrument (an autofluorescence nephelometer) will strike cloud molecules in the atmosphere. The instrument will then examine the scattered light for more information about the size, shape and concentration of the molecules. If the molecules are organic, they may glow or autofluoresce.
India plans to send its first mission to Venus no earlier than 2028, following several missions looking to compare planets in the solar system: three Chandrayaan space missions to the moon (2008, 2019 and 2023) and the Mars Orbiter Mission to the Red Planet in 2014. The Venus Orbiter Mission, nicknamed Shukrayaan, costs $147 million (12.36 billion rupees) and has been delayed from a launch in 2023.
In background information about the mission, the Indian Space Research Organisation says that Venus is particularly interesting because of its thick carbon dioxide atmosphere, high-pressure surface and active ionosphere (upper atmosphere) that's influenced by the solar wind, or constant stream of particles from the sun.
The Venus Orbiter Mission is supposed to orbit the planet to study its surface, atmosphere, and solar interactions, and will also test aerobraking in the atmosphere. Some of the science objectives of its 16 payloads include high-resolution mapping of the surface, looking at dust and "airglow" in the atmosphere, examining below the surface and looking at the X-ray spectrum of solar rays near the planet.
Particle physicists, astronomers, and cosmologists have built massive underground detectors, launched satellites, and even proposed entire new particles — all in pursuit of this elusive substance.
This quiz will test your knowledge of the strange, shadowy realm of dark matter. We'll explore the history of its discovery, the theories that try to explain it, and the cutting-edge experiments designed to catch it in the act.
Whether you're a seasoned space nerd or just curious about the universe's biggest mystery, you're in for a brain-bending ride.
Try it out below and see how well you score!
Spiral galaxies are among the most striking and familiar structures in the universe. Characterized by graceful, winding arms that spiral out from a bright central bulge, these systems are rich with both young and old stars, swirling gas and cosmic dust.
The Milky Way, our own galactic home, is one such spiral, and studying other examples like NGC 3370 provides astronomers with clues about how galaxies form and evolve.
Spiral galaxy NGC 3370 is located 90 million light years away in the Leo constellation.

NGC 3370 is home to two types of celestial landmarks that have helped astronomers chart cosmic distances with precision: Cepheid variable stars and Type la supernovas. Cepheids are pulsating stars whose brightness rises and falls in predictable cycles, the longer the period of pulsation, the more luminous they are. Meanwhile, Type la supernovas occur when a white dwarf star undergoes a thermonuclear explosion, reaching nearly the same peak brightness each time.
By comparing how bright these objects appear from Earth with how bright they actually are, astronomers can calculate their distances, and in turn, measure how quickly the universe is expanding. Together, these "standard candles" form the backbone of the cosmic distance ladder, a framework that has shaped our modern understanding of cosmic scale and motion.
You can learn more about the Hubble Space Telescope and galaxy formation.
]]>Jupiter will be visible as a bright point of light roughly 30 degrees high in the eastern sky at 12:13 a.m. EST (0513 GMT) on Nov. 5. During this time, the shadows of both moons will be visible darkening the Jovian disk as it shines below the bright "twin" stars Castor and Pollux in the constellation Gemini. Remember, the width of your clenched fist held at arm's length is roughly equivalent to 10 degrees in the night sky.
Sadly, Jupiter is too distant for the shadow transits to be spotted with the naked eye. However, a telescope with an aperture of 6-inches or more with a magnification between 100X to 150X under good atmospheric conditions will provide a good view of the shadows, while helping to resolve details in the gas giant's stormy surface.
Io's shadow will be visible darkening Jupiter's right hand side slightly below the equator as the double shadow transit gets underway shortly after midnight on Nov. 5, though eager stargazers will also be able to track it as it moves left to right across the gas giant's disk in the preceding two hours. The moon itself will also be visible to the shadow's left, sharing the same cloud band.

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Meanwhile, Europa's shadow will be visible encroaching on the extreme left of Jupiter's disk at the outset of the double transit, slightly farther from the Jovian equator. It will remain visible for a little under three hours — long after Io's umbral outline has slipped from view.
Jupiter plays host to a swarm of over 90 diverse moons, though only the largest four Ganymede, Callisto, Io and Europa — also known as the Galilean moons after famed Italian astronomer Galileo Galilei — are easily visible through an amateur telescope.
Stargazers hoping to catch a closer glimpse at Jupiter and its moons should check out our roundups of the best telescopes for viewing the night sky, while those new to the pastime may want to peruse our roundup of the best smartphone astronomy apps for navigating the post sunset realm.
Editor's Note: If you would like to share your photos of Jupiter with Space.com's readers, then please send your image(s), comments, and your name and the location of your shoot to spacephotos@space.com.
]]>Europe's Ariane 6 heavy-lift rocket took to the skies for the fourth time ever today (Nov. 4).
An Ariane 6 lifted off from Europe's Spaceport in Kourou, French Guiana today at 4:02 p.m. EST (2102 GMT; 6:02 p.m. local time in Kourou), carrying the Sentinel-1D Earth-observation satellite to low Earth orbit (LEO).
The Ariane 6 deployed Sentinel-1D about 33.5 minutes after liftoff today as planned, at an altitude of 440 miles (708 kilometers).

The Ariane 6 is the successor to the Ariane 5, which retired in July 2023 after 27 years of service. The new rocket debuted with a checkered July 2024 test flight, then followed that up with two fully successful operational launches, in March and August of this year.
Ariane 6 made it three in a row today with the launch of Sentinel-1D, which is part of the European Union's Copernicus Earth-observation program.
The Sentinel-1 series of satellites capture detailed radar imagery of Earth, "performing in all weathers, day and night," European Space Agency (ESA) officials wrote in a Sentinel-1D mission description. "This service is vital for disaster response teams, environmental agencies, maritime authorities, climate scientists — and other users who depend on frequent updates of critical data."
Three Sentinel-1 satellites had launched before today, and two of those remain operational (Sentinel-1A and Sentinel-1C). Sentinel-1D will replace Sentinel-1A, which has been eyeing Earth from orbit for 11 years — well beyond its planned operational lifetime, according to ESA.
"The Sentinel-1D satellite will work in tandem with Sentinel-1C to generate timely data," agency officials wrote in the description. "Both satellites have a C-band synthetic aperture radar (SAR) instrument on board, which captures high-resolution imagery of Earth's surface. They are also equipped with Automatic Identification System (AIS) instruments to improve detection and tracking of ships."

Today's launch was Europe's fifth orbital mission of 2025. In addition to the three Ariane 6 flights, the Vega C smallsat launcher — which, like the Arianespace, is operated by the France-based company Arianespace — has aced two missions so far this year, in April and July.
For context, SpaceX has launched 140 missions of its workhorse Falcon 9 rocket in 2025. More than 70% of those flights have been devoted to building out the company's Starlink megaconstellation in LEO.
Editor's note: This story was updated at 1:14 p.m. ET on Nov. 5 with news of successful liftoff, then again at 1:39 p.m. ET with news of satellite deployment.
]]>Discovered using the Zwicky Transient Facility (ZTF), the flare erupted from the supermassive black hole at the heart of an Active Galactic Nucleus (AGN) designated J2245+3743 and located in the center of a galaxy 10 billion light-years away from Earth. AGNs are central regions of galaxies that are dominated by feeding, or "accreting," supermassive black holes.
The supermassive black hole in J2245+3743 is feeding on surrounding gas and dust whirling around it in a flattened cloud shape called an accretion disk, but this flare is actually the result of something else: an unusually massive star venturing too close to the black hole which has a mass 500 million times greater than the sun). The tremendous gravitational influence of the black hole is ripping apart the star, and its stellar remains are being fed to this cosmic titan — an occurrence scientists call a tidal disruption event, or TDE.
"This is unlike any AGN we've ever seen," Matthew Graham, team leader at theCalifornia Institute of Technology (Caltech) and a ZTF scientist, said in a statement. "The energetics show this object is very far away and very bright."
The flare was first spotted in 2018 by the ZTF, with astronomers watching as it brightened by a factor of 40 over the course of a few months. At its peak, the flare was 30 times brighter than any prior black hole flare, emitting as much energy as 10 trillion suns. The previous most powerful TDE was the event nicknamed "Scary Barbie," which comes from its official designation ZTF20abrbeie.
"If you convert our entire sun to energy, using Albert Einstein's famous formula E = mc^2, that's how much energy has been pouring out from this flare since we began observing it," K. E. Saavik Ford, team member and City University of New York (CUNY) Graduate Center researcher, said in the statement.
This black hole flare is continuing to fade, and that indicates to the researchers that it is still swallowing the unfortunate star that ventured too close to it, which is estimated to have had an initial mass of 30 times that of the sun (for comparison, the star being devoured in the Scary Barbie event is thought to have just three to 10 times the mass of the sun).
As Graham colorfully puts it, the ongoing nature of the flare in J2245+3743 is akin to "a fish only halfway down the whale's gullet."
Helping the team continue to study this flare is the fact that the gravity surrounding supermassive black holes is so great that time itself runs slower as you get closer to the outer light-trapping boundary, or "event horizon."
"It's a phenomenon called cosmological time dilation due to the stretching of space and time. As the light travels across expanding space to reach us, its wavelength stretches as does time itself," Graham said. "Seven years here is two years there. We are watching the event play back at quarter speed."
This time dilation effect is exactly why long-term surveys like that conducted by the ZTF are so useful.
The J2245+3743 flare is of scientific interest for another reason. Astronomers have spotted around 100 TDEs thus far, and most haven't occurred in an AGN. This could be because the natural activity of supermassive black holes and the emissions that come from the accretion disk around them can camouflage TDEs. That makes TDEs around already feeding black holes tougher to spot than those involving quiet non-feeding supermassive black holes. But the huge size of J2245+3743 made it more conspicuous than most AGN-based TDEs.
Even so, this black hole flare didn't immediately present itself as something special to the team. It wasn't until 2023, five years after it was initially sighted, that data from the W. M. Keck Observatory in Hawaii revealed the extremely energetic nature of this flare.
At first, it was also important to establish that this extreme object was truly this bright and with energy escaping in all directions, not just directed straight at Earth. The team ruled this possibility out using data from NASA's retired Wide-field Infrared Survey Explorer (WISE).
The team also ruled out a massive supernova explosion as the cause of this flare, thus confirming this to be the brightest black hole flare ever detected and indicating it represents a TDE involving an exceptionally massive star.
"Supernovas are not bright enough to account for this. Stars this massive are rare, but we think stars within the disk of an AGN can grow larger," Ford said. "The matter from the disk is dumped onto stars, causing them to grow in mass."
The discovery of this powerful flare indicates that such events could be occurring across the cosmos, just waiting to be uncovered. The team will continue to go back through ZTF looking for similar events while awaiting data from the Vera C. Rubin Observatory, which could also find usually powerful TDEs.
"We never would have found this rare event in the first place if it weren't for ZTF," Graham concluded. "We've been observing the sky with ZTF for seven years now, so when we see anything flare or change, we can see what it has done in the past and how it will evolve."
The team's research was published on Tuesday (Nov.4) in the journal Nature Astronomy.
]]>Latvia will become the latest country to join the Artemis Accords, the country announced at the end of October. The European nation was the fourth commit during that month, doubling the number of countries that had previously signed the accords in 2025.
Also adding their name to the accords in October were the Philippines, Malaysia and Hungary. They were preceded by Senegal, Norway, Bangladesh and Finland, who signed earlier this year.
"Latvia’s accession to the Artemis Accords is a significant step towards our more active participation in the global space community," Latvian officials said in an Oct. 31 statement on a government-affiliated website. "We are proud to become part of a group of nations committed to exploring and using space responsibly and sustainably."
October also marks five years of the Artemis Accords, which NASA, the U.S. State Department and seven other founding nations established in 2020 as a set of international principles to designed to guide how countries explore the moon and deep space. They parallel concepts from the 1967 Outer Space Treaty, which aimed to promote peaceful cooperation in space.
Despite their name, the accords aren't directly associated with NASA's current push to return astronauts to the moon with the Artemis program. The agency is gearing up for the launch of Artemis 2 as early as February 2026, which will be the first mission to fly astronauts to the moon since 1972.
Artemis 3, currently targeted for 2027 or 2028, will be the program's first mission to land astronauts on the lunar surface, and will be followed, NASA hopes, by a series of missions to establish a permanent human presence on the moon.
Building on the strong relationship between President Trump and Prime Minister Orbán, I’m proud to expand America’s space partnership with Hungary. 🇺🇸 🇭🇺Their decision to join the Artemis Accords affirms a shared commitment to peaceful, transparent exploration—at a time when… pic.twitter.com/G9VmB2cxUGOctober 22, 2025
NASA Acting Administrator Sean Duffy announced the addition of Hungary to the accords via social media on Oct. 22 and did the same with the Philippines and Malaysia today (Nov. 3).
Latvia's announcement indicates that the country "plans" to join the accords, according to the English translation of the release, but its official inclusion may have been delayed with the U.S. government shutdown still underway. NASA officials have indicated that a formal signing ceremony will likely take place once the government reopens.
]]>Shooting stars are seen when shards of ancient comets collide with Earth's atmosphere at tens of thousands of miles per hour, which swiftly burn up in a magnificent display as they're overwhelmed by the friction created by collisions with air molecules in the atmosphere. The Southern Taurids are known for producing spectacular fireballs, as particularly large pieces of interplanetary debris can slam into our planet that can produce meteors that can momentarily turn night to day as they flare to life in the night sky.
2025 happens to be a "swarm year" for the Southern Taurids, which could see the shower put on a particularly impressive show during the Nov. 4-5 peak, when up to 10 bright meteors may be visible each hour, sharing the skies with a near-full moon. However, the light from the moon may mean that only the brightest meteors will be visible.
Swarm years are thought to occur as Earth passes through a region of Encke's debris trail containing a mass of particularly large commentary fragments. "We encounter these larger meteors about twice a decade at irregular intervals," American Meteor Society expert Robert Lunsford told Space.com in an email. "Normal Taurid particles are usually the size of pea gravel with a few larger particles mixed in. The swarm particles are only the size of baseballs up to basketballs, but will appear as fireballs from the ground instead of normal meteors."

A good time to look out for Southern Taurid meteors is in the hours following midnight on the days surrounding the shower's peak, according to EarthSky.org. Shooting stars associated with the shower will be visible streaking away from a point of origin called a radiant located in the constellation Taurus, which rises above the horizon shortly after sunset and climbs to its highest point in the southern sky in the hours following midnight.


Looking for a reliable, high quality camera with which to capture a Taurid fireball? We rate the Nikon Z8 as the best overall camera out there! Be sure to check out our Nikon Z8 review for a more in-depth look at its capabilities.
Try to allow 30 minutes for your eyes to fully adjust to the dark - while attempting to avoid staring directly at the moon - and pick out a patch of sky 40 degrees above the constellation Taurus, where the meteor trails will be the longest. Remember, the width of your clenched fist held at arm's length accounts for roughly 10 degrees in the night sky.
Lunsford notes that Earth is passing through the outer edge of the swarm during the 2025 Southern Taurid peak, which will likely provide a less spectacular show compared to the previous swarm event in 2022. "So far though, fireball activity in October has been higher than normal, indicating that we may have underestimated the strength of this year's display," continued Lunsford. "Too bad a full moon occurs during the prime portion of this display. "
The next Southern Taurid swarm isn't due to occur until 2032, so be sure to look up on Nov. 4-5 for a chance to catch a spectacular natural light show. Astronomers interested in capturing a fireball as it streaks through the night sky should read our guide to imaging shooting stars, along with our roundups of the best cameras and lenses for astrophotography.
Editor's Note: If you would capture a photo of a Taurid meteor and want to share it with Space.com's readers, then please send your image(s), comments, name and location to spacephotos@space.com.
]]>The team of astronomers suggesting this idea, led by Cambridge University's Lola Dunhaive, recently pointed the James Webb Space Telescope (JWST) at 272 small galaxies, dating back to between 800 million and 1.5 billion years after the Big Bang. The universe was still very young (in astronomical terms) when the light from these galaxies began its journey to our corner of the cosmos; now that this light has arrived to the JWST's eye, scientists saw the faraway galaxies looking dramatically different from the mature, sedately rotating disks we see in the nearby universe.
"Early galaxies were more turbulent, less stable, and grew up through bursts of star formation," Cambridge University astronomer Sandro Tacchella, a coauthor of the recent study, said in a statement.
Dunhaive and her colleagues used the JWST's NIRCam instrument to watch how ionized hydrogen gas moved around in each galaxy. In most of the subjects, instead of circling the galaxy's center in a single smooth current, gas was flowing in all directions, creating turbulent eddies, shock waves and uneven clumps of matter.
The galaxies we can see in the nearby universe are more modern, and most of them are neatly structured disks and spirals, where all the gas and stars move in the same direction around the center — unless they've suffered a recent collision or near-miss with another galaxy, anyway. But the farther astronomers peer back in time, the messier things get.
Dunhaive and her colleagues describe the galaxies in their study as existing at "the dawn of disks, where galaxies start to be sustained by rotation but will go through several episodes of instability … before settling into the cold disks we observe in the local universe." (Same, galaxies. Same.)
The JWST showed Dunhaive and her colleagues how their sample of distant galaxies looked when the universe was between 800 million and 1.5 billion years old. That's near the end of the period known as Cosmic Dawn (50 million to 1 billion years after the Big Bang), when the first stars and galaxies formed — and just on the brink of the period known as Cosmic Noon (2 to 3 billion years after the Big Bang), when bursts of new stars were lighting up the universe at a higher rate than at any time before or since. The messy little galaxies in Dunhaive and her colleagues' study were ramping up their star formation to the dramatic fireworks of cosmic noon, and that's part of why things in those galaxies were so turbulent.
Newborn stars, like newborn humans, are prone to tantrums. For a star, that means scouring the surrounding space with powerful stellar winds of charged particles, along with blasts of high-energy radiation, especially in the ultraviolet wavelengths. That makes the space in stellar nurseries (huge clouds of cold gas where new stars are forming) turbulent and chaotic. Adding to the chaos, models and observations tell us that in those early galaxies, star formation tended to happen in irregular, dramatic bursts.
These galaxies were also flailing their way through adolescence at a time when the clouds of gas suffusing the universe were much denser than they are today. After all, the universe has been inflating since the Big Bang, so it was technically a much smaller place just before Cosmic Noon – but with the same amount of matter. That fact had a huge impact on the young galaxies, because it meant that intergalactic gas was flowing — and sometimes rushing — into the young galaxies, stirring up turbulence in the process. And the supermassive black holes at the heart of each galaxy were ravenously feasting on all that gas and belching out relativistic jets of matter and radiation.
And most of the galaxies in Dunhaive and her colleagues’ study were tiny compared to the ones in our nearby universe: between 100 million and 10 billion times the mass of our sun (our Milky Way weighs in at about 1.5 trillion solar masses).
That means that things like supermassive black holes, incoming rivers of gas and bursts of star formation had an outsized impact on their stability. In other words, it was a weird time, and these young galaxies just had a lot going on.

The astronomers noticed a few exceptions: early galaxies that, for some reason buried in the stochastic processes of their pasts, managed to pull themselves together a little earlier than their peers. Those galaxies tended to be larger than average, which probably made them more resilient in the face of cosmic disruption. But most galaxies in the study were clearly still going through their messy phase.
A few previous studies have spotted some of those precocious galactic outliers, but astronomers couldn't be sure whether they were normal. Models and simulations suggested that they shouldn't be; instead, early galaxies were predicted to be turbulent, clumpy messes. Now, astronomers know the messy reality of early galaxies seems to line up well with physicists' mathematical models of how the universe works.
For Dunhaive and her colleagues, the next step will be to combine their recent observations of hot, ionized hydrogen gas with upcoming observations of cold gas and dust in the same distant, early galaxies. That will reveal more about the galaxies’ structure and evolution.
"With more data, we'll be able to track how these turbulent systems grew up and became the graceful spirals we see today," said Tacchella.
The team published the new findings on Oct. 22 in the journal Monthly Notices of the Royal Astronomical Society.
]]>Developed by Shape Shop, it's a semi-procedural open-world game that rewards player expression and flexible problem-solving skills as it tasks you to build Martian delivery systems through Lego-like pieces. That might sound quite complicated and overwhelming, but Mars First Logistics is anything but. I play a lot of games, and Mars First Logistics might be the most chill one I've come across in a long time.
Should you choose to accept this cel-shaded mission to Mars, your objective is simple: to help the Martians (that is, humans trying to colonize the Red Planet, not aliens) with — quite literally — all the heavy lifting. Your tools? Fully customizable rovers that you can build from scratch and alter to your heart's content. It's an equal parts silly and rather stimulating experience that's unlike anything I've played this year.
Though you can “finish” the game and 100% a list of achievements, I'm inclined to say Mars First Logistics is a bit of a “forever game” for those who enjoy its pitch: To roam the procedurally-generated surface of Mars helping with, you guessed it, logistics through creativity... or lots of patience. Each mission you complete will unlock credits and new parts to help you build even more outlandish designs to tackle even more difficult routes.
It's possible to complete the game without delving into the custom modifications too much, though you'll have to make good friends with the "reset vehicle position" button as the default builds have a nasty habit of falling down ravines and getting stuck between rocks in a sort of mechanised version of 127 Days. But also, you're doing it wrong. This game isn't about the missions; it's quite literally about the journey, and the wacky machines that you assemble to undertake it.
Mars' rugged terrain and the other obstacles are only as problematic as you allow them to be. Though earning credits to get more pieces can be a lengthy process, you've got enough freedom to put the more difficult tasks on hold until you can pay for the bricks and parts you need to manifest. Before you know it, that object that looked too big to possibly move is on the back of your bonkers new creation.

The deliveries you make will often lead to new infrastructure on Mars, some of which you can even construct yourself. Working on new buildings and structures that you can just plop down and/or remove also helps with the more complex objectives, especially when there are kilometers to cover between you and the destination.
Roads and monorails sound like simple enough solutions to most transportation problems past a certain point, but power lines and water pipes — among other things — add even more possibilities to the mix.
While easy to pick up, I'd have to warn the uncurious here: Mars First Logistics doesn't make the creative element optional. That's the double-edged sword of Mars First Logistics: It's very welcoming to newbies at first glance, but the true enjoyment it offers is tied to the creativity (and effort) of the driver behind the wheel.
Sure, a simple mining quest can be completed with a premade blueprint and minimal customization (or even someone else's design, as there's full Steam Workshop support), but thinking outside the box results in surprising adventures and struggles that are rewarding to overcome. If you're having a smooth brain day and those creative juices aren't flowing, you can play the game in co-op and put the old adage "two heads are better than one" to the test.

Other creativity sandbox builders like Minecraft offer a bunch of other activities and distractions that let players sidestep the "spend 3 days building a 1:1 scale replica of the Taj Mahal" side of the game. Not so here; Mars First Logistics is a physics puzzle to be solved ad infinitum. If that's your bag, you're going to love it, but if not, maybe it's time to hop on the rocket back to Earth.
I came into this game expecting a sort of Martian Truck Simulator, and while you can certainly truck your way across the red sands, accompanied by some chill tunes and with cargo in tow, that's not what I got. Instead, I found a deeply entertaining test of my mental prowess that expects your best, but gives the best back in reward.
Approached as a purely creative tool and testing ground for toy-like ideas that are grounded in science, I can even see the educational potential of Mars First Logistics. As many developers struggle to reach the highs of past sandbox legends like Kerbal Space Program, Shape Shop's ambitious physics sim instantly takes off and lets our imaginations run wild.
'Mars First Logistics' is available now for purchase on PC (Steam). A code was provided by the developer for this article.
]]>On Oct. 28, Hurricane Melissa became the fourth hurricane in 75 years to make landfall on the island of Jamaica and shattered several Atlantic hurricane records. It is now tied with the 1935 "Labor Day" hurricane for the strongest Atlantic hurricane to make landfall on record, according to Yale Climate Connections. As of Oct. 31, at least 50 deaths have been reported in the storm's wake, and total damages could reach over $50 billion, according to Reuters. The full impact of the storm is still being assessed.
Satellite photos released by Vantor Technology (formerly Maxar) are beginning to reveal the extent of the damage left in Melissa's wake, which left the island of Jamaica unrecognizable in many parts. Vantor Technology recently shared imagery on X showing several locations throughout the island nation that flooded or were damaged by high winds brought by Hurricane Melissa.
Following Hurricane Melissa, Vantor made its satellite imagery available for free in order to help rescue and recovery efforts. "This imagery can be used by frontline organizations and geospatial community members to map changes on the ground and identify the most severely impacted areas, helping ensure resources are allocated quickly and effectively," Vantor wrote alongside the images.

Imagery like this is useful to first responders and other organizations on the front lines as it can help them locate where the hardest hit areas are and where immediate help is needed most. And as the flood waters begin to recede, responders can also use satellite imagery to determine when it's safe to get into those areas to search for survivors and survey the damage.

There were only two hurricanes before Melissa, Hurricane Charlie and Hurricane Gilbert, that reached the status of a major hurricane on the Saffir-Simpson Hurricane Wind Scale when they made landfall on Jamaica.

But Melissa surpassed every Jamaican hurricane and is now ranked as the strongest ever to landfall on the island, reaching a Category 5 storm last week with sustained winds at 185 miles per hour mph (298 km/h).
]]>You can get 20% off all Unistellar smart telescopes from now until the end of November.
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Humanity's drive to explore has taken us across the solar system, with astronaut boots, various landers and rovers' wheels exploring the surfaces of several different planetary bodies. These environments are generally hostile to human and equipment health, so designing and executing these missions requires a lot of planning, testing and technological development.
You may have heard about the extensive testing facilities for spacecraft and equipment, but how do scientists prepare for the human aspect of space exploration?
One way to test out techniques and identify situations that may arise during a real mission is using a simulation, which in this field is more commonly known as an analog. Researchers choose and design analog missions and environments to replicate elements of a real mission, using what is available here on Earth.
These missions are conducted in extreme environments on Earth that are comparable to the moon or Mars, in habitats designed to replicate living quarters, or a combination of both. Researchers can use analogs to study crew performance and procedures, or to test instruments under development for use in space.
For example, operating a drill or wrench may seem easy here on Earth, but try doing the same task in thick gloves on a bulky, pressurized space suit in lower gravity. Suddenly, things aren't so straightforward. Testing these scenarios on Earth allows researchers to identify necessary changes before launch. The analogs can also train crew members who will one day undertake the actual mission.
I'm a planetary scientist, which means I study the geology of other planets. Currently, I study environments on Earth that are similar to other planets to improve our understanding of their counterparts elsewhere in the solar system. I participated as a volunteer in one of these analog missions as an "analog astronaut," serving as the crew geologist and applying my prior research findings from studying the surfaces of the moon and Mars.
These analog missions vary in setting, length and intensity, but all aim to learn more about the human factors involved in space exploration.
Analog missions are designed to simulate the crew's experience in a given mission plan. In some cases, they simulate surface operations on the moon or Mars for up to a year. Others might replicate the experience of being in transit to Mars for a period of time, followed by the crew "landing" and exploring the surface.
NASA uses several analog mission facilities spread across the world. For example, the Mars Desert Research Station in Utah is located in an environment chosen to imitate conditions on Mars, while analog missions at Aquarius, an undersea research station off the coast of Florida, help scientists learn about crew behavior and psychology in a confined habitat located in a hostile environment.
Some natural environments are commonly used for analog operations, such as volcanic terrains in the western U.S., human-made craters in Nevada, the natural meteor crater in Arizona and research stations in Antarctica. These locations mirror the geologic settings the crews are likely to encounter on future missions, and so training in these locations helps them execute the actual missions.
I participated in a simulated 28-day lunar surface mission at a facility called Hi-SEAS as part of a study on crew dynamics and psychology in extreme isolation. The facility is located on Mauna Loa, a volcano on the big island of Hawaii. This habitat has been used for a variety of studies, as the volcanic terrain is reminiscent of both the moon and parts of Mars, and the isolated location simulates being in space.

Most missions require applicants to hold relevant degrees. They must undergo physical health and psychiatric evaluations, with the goal being to select individuals with similar backgrounds to those in the astronaut corps. The ideal crew is typically made up of participants who work and live well with others, and can stay cool under stress.
Crews also include at least one person with medical training for emergencies, as well as a variety of scientists and engineers to operate the habitat's life support systems.
The experiences of each crew varies, depending on the mission design, location and makeup of the crew. My mission was designed so that the six crew members would not have any information about our crewmates until we arrived in Hawaii for training. In addition to geology expertise, I also have some medical training as a Wilderness First Responder, so I was there to assist with any medical issues.

Once in Hawaii, the crew spent three days learning how to operate the habitat systems, including the hydroponic garden and solar panels. We practiced emergency procedures and were taught how to perform other tasks.
After that orientation, we were deployed to the habitat for 28 days. We turned in our phones to mission control and could only access the internet to check emails or use a few preapproved websites required for our daily duties. Our days were scheduled with tasks from wake up, about 6:30 a.m., to lights out, about 10 p.m.
The tasks included a variety of exercises to assess individual and group performance. They included individual assessments – similar to a daily IQ test – and group computer-based tasks, such as team 3D Tetris. The researchers remotely monitored our interactions during these activities, and the results were analyzed as the mission progressed. They used our fluctuating performance on these activities as a proxy for estimating stress levels, group cohesion and individual well-being.
Additionally, we went on two-to-three-hour extra-vehicular activities, or excursions outside the habitat, on alternating days. During these expeditions, we conducted geologic investigations on the volcano. On our "off days," we spent two hours exercising in the habitat. We had to be fully suited in a mock spacesuit any time we went outside, and we had to be careful about the airlock procedures. We were never outdoors alone.
We could only eat freeze-dried and powdered foods, aside from what we were able to grow in the hydroponic system. We had no additional food delivered during our stay. Water was also rationed, meaning we had to find innovative ways to maintain personal hygiene. For example, a bucket shower one or two times per week was allowed, supplemented by "wilderness wipe" baths. As someone with a lot of very curly hair, I was happy to figure out a method for managing it using less than two liters of water per week. We were also permitted to do laundry once during our stay, as a group. Sorting through your crewmates' wet clothes was certainly one way to bond.
Though physically demanding at times, the workload was not unreasonable. We were kept busy all day, as certain everyday tasks, such as cooking, required more effort than they might need in our normal lives. Preparing nutritionally balanced and palatable meals while rationing our very limited resources was hard, but it also provided opportunities to get creative with recipes and ingredients. We even managed to bake a cake for a crew member's birthday, using peanut butter protein and cocoa powders to flavor it.
After dinner each night, we shared the pre-saved movies and shows we had each brought with us into the habitat, as we could not access the internet. Those of us who had brought physical copies of books into the habitat would trade those as well. One crew member managed to acquire a downloadable form of the daily Wordle, so we could still compete with our friends back home. We also played board games, and all of these activities helped us get to know each other.
Though different from our typical daily lives, the experience was one of a kind. We had the satisfaction of knowing that our efforts advanced space exploration in its own small way, one IQ test and slapdash cake at a time.
This article is republished from The Conversation under a Creative Commons license. Read the original article.
]]>"Two selected Pakistani astronauts will participate in training together with Chinese astronauts. One of them will be scheduled to carry out a short-duration flight mission as a payload expert," Zhang Jingbo, spokesperson for the China Manned Space Agency (CMSA), told reporters on Thursday (Oct. 30).
Zhang was speaking at a press conference at Jiuquan spaceport a day ahead of the launch of the Shenzhou 21 crewed mission. Shenzhou 21 launched on Friday (Oct. 31), sending commander Zhang Lu and rookie astronauts Wu Fei and Zhang Hongzhang to Tiangong.
China and Pakistan signed a cooperation agreement on sending an astronaut to Tiangong in February of this year. A preliminary astronaut selection round is currently being conducted in Pakistan, while the secondary and final selections will be carried out in China, according to Zhang.
"During the flight, in addition to performing the crew's daily duties, they will also undertake scientific experiments for Pakistan," Zhang explained.
Zhang did not state on which mission the Pakistani astronaut will fly. When that happens, they will take one of three seats aboard a Shenzhou spacecraft, launching on a Long March 2F rocket from Jiuquan in the Gobi Desert. Shenzhou 22 is set to launch in around six months time, with the crew replacing the Shenzhou 21 astronauts aboard Tiangong. Shenzhou 23 will launch about one year from now.
Although CMSA has not confirmed details, the short-duration nature of the international astronaut visit suggests that the Pakistani astronaut will fly to Tiangong aboard a Shenzhou spacecraft with two Chinese crewmates, stay aboard the station for a number of days, then return to Earth with two of the three crewmembers from the previous mission, who will have completed their customary six months in space. That would leave one Chinese astronaut to complete the country's first full one-year stint aboard Tiangong in a continuous stay.
The Tiangong space station is a three-module orbital outpost that was completed in late 2022. China aims to keep the space station operational and permanently occupied for at least a decade, with the facility expected to outlive the much larger International Space Station. Pakistan also partners with China on the latter's International Lunar Research Station, planned for construction in the 2030s.
]]>The Bwine F7GIM is something of an oddball in terms of weight because at 12.6 oz / 357 g it will require registration with the FAA in the U.S, even for recreational use. The focal length of the camera is 60 mm, which means you can capture subjects from further away, which works well given the weight. Put simply, you don’t have to fly as close as with a 24 mm equivalent camera.
Weight: 12.6 oz / 357 g
Dimensions: 6.50 x 3.54 x 2.56 in / 165 x 90 x 65 mm folded / 14.17 x 11.02 x 2.56 in / 360 x 280 x 65 mm unfolded
Battery: 3200 mAh Li-ion / up to 35 minutes flight
Charger type: USB-C cable
Modes: Stable (Camera), Sport
Video transmission range: 1.89 miles
Video resolution: 4K, 2.7K, 2K, 720p (720p stored on phone)
Frame rates: 4K 30 FPS, 2.7K 50/30 FPS, 2K 50 FPS, 720p 30 FPS
Image quality is respectable, and you can capture photos in JPEG format up to 5700 x 3200 px, which equates to 18MP. Video can be captured up to 4K 30 FPS, while reducing the capture resolution to 2.7K and 2K allows for 50 FPS capture. This is all pretty standard for a basic drone like this, which also offers a handful of useful features we’ll cover later.
The drone is perfectly adequate in most ways, but it is on the expensive side considering the other drones are available for a similar price. These include the DJI Neo and the Potensic Atom 2, both of which are superior drones. However, the F7GIM could still be exactly what you’re looking for, and it does excel in one or two areas, including wind resistance.

This is a compact folding drone that’s just 6.50 x 3.54 x 2.56 in / 165 x 90 x 65 mm when folded and 14.17 x 11.02 x 2.56 in / 360 x280 x 65 mm when unfolded. Looking at it, you could easily mistake the F7GIM for being a sub-250 g model, but it sneaks in at a weight of 12.6 oz / 357 g. As previously mentioned, this means it has to be registered with the FAA in the United States. The drone does feature Remote ID, making it FAA-compliant.
The weight of the F7GIM certainly isn’t the end of the world, but it is something to consider if you’re only looking for a drone for recreational flight. Many beginners opt for sun-250 g models precisely because of not having to register. Not to mention, they’re also smaller and lighter to carry around.



Getting back to the design, the drone comes in a dark grey with orange accents on the propellers, which does look good. Build quality can’t be faulted, while the camera and 3-axis gimbal are well-made.
There’s also an optical flow sensor on the bottom of the airframe for detecting the ground during low-level flying and to assist with landing. As you’d expect, there’s no collision avoidance.


The controller is of a reasonable quality and is quite chunky and comfortable to hold thanks to rubberized grips. It features a small screen that shows basic information, but it’s not bright, so it can be difficult to view in sunny conditions.
The controller offers a range of direct access controls, and the control sticks can be stowed at the bottom of the controller for transportation and storage. The phone holder extends from the top of the controller with space to store the phone cable when not in use.

The F7GIM comes with a level 5 wind resistance rating, which equates to wind speeds of up to 24 mph. The drone was tested in winds of this speed and it had no issues whatsoever, although this is the same wind resistance level as many lighter sub-250 g models. With the weight increase, a power increase would be welcome, but it’s unfortunately absent.
Flying in winds of around 25 mph provided flight times of around 22 minutes, as opposed to the advertised 35 minutes, but it’s safe to assume that less windy conditions would provide longer flights. This would most likely be just a few additional minutes rather than the full advertised 35 minutes per battery, which is optimistic at best.
The F7GIM features GPS and Return to Home (RTH) functionality, and you can set the RTH altitude within the Bwine Mini app. By default, this is set to the minimum of 20 m, so be aware of your surroundings when making your first flight and adjust accordingly.
Return to Home can be initiated by the pilot when the battery is low and when the controller connection is lost. Smart RTH allows you to also control the drone during the return process to avoid obstacles.
There are a few basic subject tracking functions available, but during testing these weren’t the best examples I’ve experienced. The GPS follow was the most reliable since it tracks the controller, but the subject doesn’t always remain in the centre of the camera frame. Orbit, where the drone orbits the subject, was unreliable and haphazard.
Despite these features lacking in performance, overall flight performance is great and can’t be faulted. The controller allows for precise movements, and the gimbal is smooth when incorporating gimbal movements with flight to capture interesting video footage. This is always a good test of drone gimbals, and the F7GIM passed with flying colors.
Within the main feature menu, there are also quite a few other options, including Route Planning, VR Split Screen, Digital Zoom, Night Mode to increase brightness in the app camera view and several other options.
The Bwine Mini app is basic and easy to use, which is ideal for beginners. One point to mention is that by default, the drone is set to Beginner Mode, which limits altitude and flight distance, so you’ll have to manually switch this off to increase both of these.





The F7GIM camera features a 1/3.2 in Sony sensor with a 60mm equivalent focal length and an f/2.0 aperture. This is a long focal length for a single-camera drone, but it seems to work. The camera is supported by a 3-axis gimbal, resulting in smooth video capture.
The important point to make here is that the camera is fully automatic with fixed focus, so you have no control over any settings. This is perhaps ideal for photography beginners, but less so for enthusiasts.

Image quality is surprisingly good despite the fully automatic camera, although it does have a depth-of-field issue. Objects closer to the camera are lovely and sharp, but those in the distance do fall out of focus.
The centre of the frame is also characteristically sharper than the outer area, which is normal for most drones, and since the camera is automatic, it’s best to shoot with the sun behind the drone for more reliable exposures. With no control over exposure compensation, shooting towards the sun results in underexposure.
The only variables that can be changed are the resolution and frame rate of video, while the resolution of photos can be adjusted to three different amounts. Photo sizes are in a 16:9 ratio and are captured in JPEG format. The resolutions available include 3840 x 2160 px, 4096 x 3072 px and 5700 x 3200 px.
Video can be captured in 4K 30 FPS, 2.7K 50/30 FPS, 2K 50 FPS and 720p 30 FPS. 720p is stored on your phone, alongside photos, so you have to keep an eye on how much storage it’s using over time. It’s a shame this can’t be switched off if desired. Other footage and photos are stored on the microSD card in the drone, and the F7GIM can accept 16 to 128GB cards. Video quality is, as is often the case with drones, better than photo quality.
The Bwine F7GIM is a respectable beginner drone, but where it ultimately falls is in its price of $400 / £296. This puts it in direct competition, price-wise, with the DJI Neo and the Potensic Atom 2, which are both more advanced drones with superior flight performance and features in general.
If the F7GIM was less expensive, it would be a much more attractive proposition, although it’s not a bad drone at all if you’re willing to pay that price. Like all tech, it depends on what you're looking for in terms of brand and features.
The drone comes in a kit which includes the drone, controller, two batteries, an extra set of propellers, an extra set of controller sticks, phone cables, USB-C cables for charging, a carry case and other accessories. This is everything you need to get started.
This is a tricky one because the F7GIM is a good beginner drone. It flies well, image quality is good for a basic model of this type and the fully automatic camera makes it incredibly easy to capture photos and videos. What’s more, the kit comes with everything you need and more in terms of the accessories that are included.
The main issue is the price, which is too close to bigger-name and more advanced drone models. However, if price isn’t an issue for you, you won’t go wrong with the F7GIM. It may be the simplicity of the camera that attracts some people to it because it’s very much a point-and-shoot affair.
The DJI Neo is a sub-250 g beginner drone that can be flown autonomously with impressive subject tracking functionality, with the DJI Fly app via your smartphone or using a traditional controller. The drone can capture 4K video and photos in JPEG format.
The Holy Stone HS900 Sirius is another sub-250 g beginner drone worth considering, thanks to excellent flight performance, impressive image quality and useful features. Video can be captured up to 4K and photos in Raw and JPEG.
The Potensic Atom 2 is the best DJI alternative available in a regulator-friendly sub-250 g package. This impressive drone is available at an attractive price and can capture 4K video and photos in Raw and JPEG.
]]>By the time that the International Space Station (ISS) is safely and deliberately de-orbited over the Pacific Ocean, the station will have been permanently crewed for 30 years — it has had visitors ever since the first Expedition 1 mission (consisting of one astronaut and two cosmonauts) first docked with the fledgling, half-built station on November 2, 2000. Yet as we begin to near the end of the ISS's time in low Earth orbit, we are beginning to think ever more about the station's true legacy, whether it achieved what it set out to achieve, and what we will lose when it is finally gone.
The loss of the ISS will be keenly felt by many; it will be like when one of our beloved Mars rovers falters and is forced to end its mission. Sure, there will be other Mars rovers after, but they will be different. There will be other space stations, but they will be different.
For some, though, says sociologist Paola Castaño-Rodriguez of the University of Exeter, the end of the ISS will be no loss at all, as they always saw it as a white elephant.
"When it comes to spaceflight, everybody uses the word 'we,' but when you're a sociologist, the first thing you ask is, who is 'we?'" she told Space.com. "Just as equally as you have enthusiasts, there's a lot of people for whom this is an obscene waste of money."
Castaño-Rodriguez studies the processes by which science is conducted on the ISS, the unique way in which people from across the world come together to perform this science, and the different criteria by which this science is valued. She's also currently working on her book, "Beyond the Lab: the Social Lives of Experiments on the International Space Station," which explores these topics through the stories of three science experiments: the first time lettuce was grown on the ISS, the twin experiment involving Mark and Scott Kelly, and the Alpha Magnetic Spectrometer particle physics experiment affixed to the exterior hull of the ISS.
The critics are correct that the ISS is expensive, having cost $150 billion to build and operate so far, with NASA alone spending $3 billion per year to maintain it. For that amount of money, it doesn't seem unreasonable to expect some major outputs. Indeed, the science case for building the space station back in the 1990s was that the experiments that could be performed on the ISS could help cure cancer or discover dark matter.
"In a way, part of the problem is in how the space station was pitched, with these big promises that scientists had to make to get funded, and the issue is that those things have become the things that the space station is accountable for," said Castaño-Rodriguez.
The point is, the way we judge what we will lose when the ISS is de-orbited will differ depending on who is doing the judging — and how that judgement is cast. Looking at things purely from the eureka moments of scientific discovery that make headlines, people might consider the ISS a disappointment. Still, earlier this year, NASA has revealed that over 4,000 science experiments have been conducted on the ISS over the past 25 years, resulting in 4,400 scientific papers — but those findings have been, for the most part, relatively modest or incremental rather than revelatory.
However, looking at science in only this way would completely ignore what Castaño-Rodriguez considers to be the true success of science on the station, and what will be most keenly felt when it is lost.
"It takes for granted all the infrastructural work, all the operations, all the processes that, to me, are actually the key outcome of the space station, which is learning how to do science in such an adverse environment," she said. "In a way, it requires re-educating audiences about what is valuable about science. It's not just the shiny headline discovery, it is all the knowledge that is produced to enable a field to move forward. It's an epic and incredibly complex process to do these experiments on the space station.
"I think, when it comes to further space exploration, this infrastructural knowledge is going to be needed. There will be gaps and it is uncertain at the moment how they are going to be filled with other platforms."

Those other platforms that Castaño-Rodriguez refers to are commercial space stations NASA expects to replace the ISS. Companies such as Axiom Space, Blue Origin and a partnership of Starlab Space and Northrop Grumman have signed Space Act agreements with NASA to design and build new space stations. However, with this commercialization comes uncertainty about how much of what the ISS did will be transferred over to the new, privately developed orbiting habitats.
On the one hand, much of the expertise in these commercial ventures is from ex-NASA spaceflight people, and so rather than lose their expertise when the ISS is de-orbited, the processes and values that they embodied at NASA will be merged into the identity of the new commercial stations.
But on the other hand, commercialization could bring with it a loss of transparency.
In the United States, the direction of centrally funded science is governed by the peer review process of the National Academy of Sciences' decadal surveys. It is this process that guides what research NASA funds on the space station, which ensures that science on the ISS is judged only on its scientific merits.
"Are private companies going to be accountable to things like the decadal surveys?" asked Castaño-Rodriguez. "In terms of the process by which experiments will be selected, that's a big question, because the implication is that scientists just become the paying customers and the only experiments that go to the station are the ones that can be afforded."
Science today on the ISS is a truly public affair, with a mandate to make all the data collected by science experiments performed on the space station available in a public repository.
"This is a huge deal because you don't have to be involved in spaceflight to analyze the data," said Castaño-Rodriguez. "This open science is very much part of the space station's history that is not really talked about much, but it's a really important infrastructural aspect that is very international with researchers all over the world participating and engaging and re-analyzing the data produced on the space station."
The risk is that the transition from the publicly funded ISS to commercial stations could see the loss of this accessible open data, though Castaño-Rodriguez sees some reasons for optimism, for example through ex-NASA staff who, in the past, have championed open data and who now work for the private companies.
Castaño-Rodriguez also thinks commercial stations could be just as international as the ISS.
“They're going to be pathways to a lot of middle- to high-income nations to start paying for their astronaut missions," said Castaño-Rodriguez. For example, Axiom Space has already flown two Saudi astronauts on one of their missions (previously NASA had flown a Saudi prince on shuttle Discovery in 1985) as well as the first Turkish astronaut.
However, there's a difference between being a paying guest and a true partner, which is how the mix of international astronauts on the ISS has mostly been seen.
“I don't think [the commercial stations] will be anything like the particular international configuration of the ISS,” said Castaño-Rodriguez. "It's very much a product of its time."
That time being the 1990s and 2000s, off the back of the nearly five-decade Cold War and the dawn — arguably a false one — of renewed international cooperation both on Earth and in space. Militarily trained astronauts on both sides began shaking hands with people they'd been ideologically trained to treat as enemies. At the level of crew-member interactions, mission-control interactions, and scientific interactions, cooperation in space on the ISS helped break down barriers.

When we lose the ISS, we won't just lose its hardware, or how it made science in low-Earth orbit accessible. We'll also lose a pillar of space history that brought together people from different countries that were still learning to trust each other. Even today, despite Russia's invasion of Ukraine and tension that globally arose from the conflict, cosmonauts still fly to the station and work closely with their crewmates from other nations. It's hard to see that being replicated on a commercial station in today's geopolitical climate, at least to the same level and for such a prolonged time as it was exhibited on the ISS.
The space station really has been a unique experiment, an orbiting petri dish where humans have learned to work and live together in space. Wherever our spacefaring takes us in the future, it will owe a great deal to the legacy of the ISS. While we will lose the physical space station, Castaño-Rodriguez describes an infrastructural knowledge that will live on, at least in part, in where we take crewed space exploration next.
As part of her research, Castaño-Rodriguez has interviewed nearly a hundred astronauts, engineers and scientists involved in the ISS who have a unique insight into the importance of this orbiting science post. Perhaps the legacy of the ISS is best summed up by Sergei Krikalev, cosmonaut on the Expedition 1 mission 25 years ago.
"I asked him, when he was there on Expedition 1, did he remember any of the science experiments?" said Castaño-Rodriguez. "He looked me straight in the eye and said, 'the space station is the experiment.'"
]]>Thanks to modern technology, observatories are advancing their reach. The National Science Foundation's NOIRLab is a hub for ground-based optical and infrared astronomy, providing telescopes and data infrastructure that enable discoveries across stars, galaxies, dark matter, exoplanets and more.
One of those ground-based telescopes is the Rubin Observatory, named after famed astronomer Vera Rubin. Unlike other telescopes, the Rubin Observatory is working to capture the night sky in real-time by scanning it every few nights, creating a digital movie of our universe.
The Rubin Observatory is located on Cerro Pachón in the Andes Mountains in Chile.

To scan the skies in real time, the Rubin Observatory relies on the LSST camera, the largest digital camera ever built, that can image an area of the sky around 40 times the size of the full moon in a single exposure. As it runs, the LSST camera will produce tens of petabytes of data over the next decade. Astronomers hope to use this data to help tackle some of the most pressing cosmic questions, such as those around dark matter and dark energy or studying potentially hazardous asteroids that may collide with Earth.
Rubin's data will be made publicly available during this process, empowering scientists and even citizen scientists worldwide to explore, analyze and make discoveries about our cosmos.
You can learn more about the Rubin Observatory and other ground-based telescopes.
]]>At 5:30 p.m. EST (2230 GMT), the moon will reach its closest point to the Earth for the year, known as perigee, at a distance of 221,726 miles (356,833 kilometers). Nine hours and 11 minutes prior to that, the moon will officially turn full. It will, in fact, be the biggest Though a full moon theoretically lasts just a moment, that moment is imperceptible to ordinary observation, and for a day or so before and after most will speak of seeing the nearly full moon as "full": the shaded strip is so narrow, and changing in apparent width so slowly, that it is hard for the naked eye to tell whether that dark strip is present or on which side it is.
So, when the moon shines down on your neighborhood on Wednesday night, keep this in mind: what you're looking at is not precisely a "full" moon, but a waning gibbous moon, already many hours past its stage of full illumination.
Most media outlets love to treat this as some sort of special or unusual occurrence. Upon hearing that a specifically selected moon comes with the prefix "super" attached, people rush outside to get a look and come away thinking that they have just witnessed something akin to a rare cosmic alignment. Such feelings put a new spin on the whimsical tale penned in 1837 by Hans Christian Anderson, "The Emperor's New Clothes."
While this will indeed be the "Biggest Full Moon of 2025," the variation of the moon's distance is not readily apparent to most observers viewing the moon directly. The moon comes to perigee once, occasionally twice a month (their respective distances vary by 3% percent), but as we just noted, this one will be the closest one in 2025. Next year, on May 31, full moon will coincide with apogee — its farthest point from Earth in its orbit — and it will appear about 14% smaller (what some call a "micro-moon").
And then there is the other facet . . . the oft-told statistic that the moon is 30-percent brighter than normal. But that factors in only as a 0.2 or 0.3 magnitude difference in brightness; hardly perceptible at all to the human eye.
In fact, I once took a phone call at New York's Hayden Planetarium from a young lady who sounded like she had been cheated. "I went outside last night to look at that so-called 'super' moon and was very much disappointed. It didn't look at all brighter than normal." When I queried her on what she had expected to see, she replied, "I thought it was going to be something like those three-way light bulbs. Like when you go from 100 to 150 watts; I thought the moon was going to appear noticeably brighter last night, but it really wasn't at all!"
Of course, once somebody is told that the moon is closer-than-normal to Earth and consequently appears somewhat larger in apparent size, then they likely will respond with: "Oh yeah! It does look bigger than normal!" This is especially true if one sees the moon near the horizon, where the enigmatic "moon illusion" always comes into play. The fact that the moon will be much closer than usual on Wednesday will only serve to amplify this strange effect.
In addition, the near coincidence of this full moon with perigee will result in a dramatically large range of high and low ocean tides. Any coastal storm at sea around this time would almost certainly aggravate coastal flooding problems at high tide, or, in the case of a strong wind pushing the water offshore, it would create a very low water situation at low tide.
Such an extreme tide is known as a perigean spring tide, the word spring being derived from the German springen — to "spring up," and is not at all a reference to the spring season. Spring tides occur when the moon is either at full or new phase. At these times, the moon and sun form a line with the Earth, so their tidal effects add together (the sun exerts a little less than half the tidal force of the moon.) "Neap tides," on the other hand, occur when the moon is at first and last quarter and works at cross-purposes with the sun. At these times tides are weak.
Tidal force varies as the inverse cube of an object's distance. This month's full moon is 12.2 percent closer at perigee compared to next May's apogee full moon. Therefore, it will exert 46 percent more tidal force.
The highest tides will not, however, coincide with the perigee moon but will actually lag by one or two days, depending on the specific coastal location. For example, at Cape Fear, North Carolina, the highest tide (6.88 feet) will be attained at 7:20 a.m. EST on Thursday. For New York City, high water (6.34-feet) at The Battery comes at 7:59 a.m. EST on Thursday, while at Boston Harbor, a peak tide height of 12.22-feet comes at 11:54 a.m. EST on Friday, almost 2 days after perigee.
And yet, if the criteria for the "super" branding is chiefly dependent on the moon's arrival at its closest point in its orbit relative to the Earth, then it might be a bit of a misnomer. Indeed, the moon arrives at perigee point of its orbit every month, sometimes (as previously noted) twice a month.
Indeed, the full moons that immediately flank the full moon coinciding with perigee are now also being branded as supermoons. This year, for instance, the full moon that we had on Oct. 6 (the "Harvest Moon") was deemed "super." And so will the one next month on Dec. 4. Other years have four (such as in 2028 and 2034) and, in several cases, (as in the years 2029 through 2033) there can be as many as five!
So why can't we have a supermoon at other phases? On Feb. 24, 2026, for instance, the first quarter moon will come within less than eleven hours of perigee. But nobody ever gets excited about a "super" half-moon.
The popular astrophysicist, Dr. Neil deGrasse Tyson, probably said it best:
"In the overall scheme of things, is this relatively small increase in the moon's apparent size really so meaningful? I mean, if you turned a 14-inch pizza into a 15-inch pizza, would you then call it a "Super-pizza?"
Maybe when it comes to our natural satellite, size doesn't really matter after all.
Joe Rao serves as an instructor and guest lecturer at New York's Hayden Planetarium. He writes about astronomy for Natural History magazine, Sky and Telescope and other publications.
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