diff --git "a/nasascraper_data.csv" "b/nasascraper_data.csv" --- "a/nasascraper_data.csv" +++ "b/nasascraper_data.csv" @@ -1,190 +1,224 @@ date,explanation,hdurl,media_type,service_version,title,url,copyright,data_type,links,id,neo_reference_id,name,name_limited,designation,nasa_jpl_url,absolute_magnitude_h,estimated_diameter,is_potentially_hazardous_asteroid,close_approach_data,orbital_data,is_sentry_object,source,scrape_timestamp -2016-07-08,"At the core of the Crab Nebula lies a city-sized, magnetized neutron star spinning 30 times a second. Known as the Crab Pulsar, it's actually the rightmost of two bright stars, just below a central swirl in this stunning Hubble snapshot of the nebula's core. Some three light-years across, the spectacular picture frames the glowing gas, cavities and swirling filaments bathed in an eerie blue light. The blue glow is visible radiation given off by electrons spiraling in a strong magnetic field at nearly the speed of light. Like a cosmic dynamo the pulsar powers the emission from the nebula, driving a shock wave through surrounding material and accelerating the spiraling electrons. With more mass than the Sun and the density of an atomic nucleus, the spinning pulsar is the collapsed core of a massive star that exploded. The Crab Nebula is the expanding remnant of the star's outer layers. The supernova explosion was witnessed on planet Earth in the year 1054.",https://apod.nasa.gov/apod/image/1607/hstheritage_crabcore.jpg,image,v1,The Swirling Core of the Crab Nebula,https://apod.nasa.gov/apod/image/1607/hstheritage_crabcore1024.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2013-09-08,"What kind of cloud is this? A type of arcus cloud called a roll cloud. These rare long clouds may form near advancing cold fronts. In particular, a downdraft from an advancing storm front can cause moist warm air to rise, cool below its dew point, and so form a cloud. When this happens uniformly along an extended front, a roll cloud may form. Roll clouds may actually have air circulating along the long horizontal axis of the cloud. A roll cloud is not thought to be able to morph into a tornado. Unlike a similar shelf cloud, a roll cloud is completely detached from their parent cumulonimbus cloud. Pictured above, a roll cloud extends far into the distance as a storm approached in 2007 in Racine, Wisconsin, USA.",https://apod.nasa.gov/apod/image/1309/rollcloud_hanrahan_3072.jpg,image,v1,Roll Cloud Over Wisconsin,https://apod.nasa.gov/apod/image/1309/rollcloud_hanrahan_960.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -1998-06-30,"Scroll right and watch the universe evolve. Above is a computer simulation depicting the evolution of our entire universe. On the far left is a slice of the universe soon after the Big Bang - over 10 billion years ago. As time progresses toward the right, the initially smooth universe can be seen becoming more and more clumpy. The vertex near the far right marks the present day. The largest slice of the universe actually surveyed is simulated to the vertex's right. This artificial universe, called a Hubble Volume, was designed to mimic what humanity might see were we to have powerful enough telescopes. By comparing different computer simulations to reality, we might be able to better tell what kind of universe we live in.",https://apod.nasa.gov/apod/image/9806/compuni_virgo_big.gif,image,v1,The Universe Evolves,https://apod.nasa.gov/apod/image/9806/compuni_virgo.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2013-02-14,"On another Valentine's Day (February 14, 1990), cruising four billion miles from the Sun, the Voyager 1 spacecraft looked back to make this first ever family portrait of our Solar System. The complete portrait is a 60 frame mosaic made from a vantage point 32 degrees above the ecliptic plane. In it, Voyager's wide angle camera frames sweep through the inner Solar System at the left, linking up with gas giant Neptune, at the time the Solar System's outermost planet, at the far right. Positions for Venus, Earth, Jupiter, Saturn, Uranus, and Neptune are indicated by letters, while the Sun is the bright spot near the center of the circle of frames. The inset frames for each of the planets are from Voyager's narrow field camera. Unseen in the portrait are Mercury, too close to the Sun to be detected, and Mars, unfortunately hidden by sunlight scattered in the camera's optical system. Small, faint Pluto's position was not covered. APOD Public Talk: Feb. 21, Howard Astronomical League, Columbia, MD",https://apod.nasa.gov/apod/image/1302/ssportrait_vg1_big.jpg,image,v1,Solar System Portrait,https://apod.nasa.gov/apod/image/1302/ssportrait_vg1.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2020-08-13,"What planets are those behind that unusual rock spire? Saturn (lower left) and Jupiter.  This month, after sunset, the bright planetary duo are quite prominent toward the southeast.  Now your view of our Solar System's largest planets might not include a picturesque hoodoo in the foreground, nor the spectacular central band of our Milky Way Galaxy across the background, but should be quite eye-catching anyway.  The featured image is a composite of consecutive foreground and background exposures all taken in late May with the same camera and from the same location -- the badlands of the  Ah-Shi-Sle-Pah Wilderness in the San Juan Basin in New Mexico, USA.  The rock spire, informally dubbed 'Alien Throne', stands about 3 meters tall. Saturn and Jupiter will remain visible together after sunset for several months.",https://apod.nasa.gov/apod/image/2008/AlienThrone_Zajac_3807.jpg,image,v1,Jupiter and Saturn Rising Beyond Alien Throne Rock,https://apod.nasa.gov/apod/image/2008/AlienThrone_Zajac_960.jpg," -Marcin Zając -",exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -1995-09-07,"This Hubble Space Telescope image of a group of faint galaxies ""far, far away"" is a snap shot of the Universe when it was young. The bluish, irregularly shaped galaxies revealed in the image are up to eight billion light years away and seem to have commonly undergone galaxy collisions and bursts of star formation. Studying these objects is difficult because they are so faint, however they may provide clues to how our own Milky Way Galaxy formed.",https://apod.nasa.gov/apod/image/fbg.gif,image,v1,Distant Galaxies,https://apod.nasa.gov/apod/image/fbg.gif,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2022-07-17,"What are those spots on Jupiter? Largest and furthest, just right of center, is the Great Red Spot -- a huge storm system that has been raging on Jupiter possibly since Giovanni Cassini's likely notation of it 357 years ago. It is not yet known why this Great Spot is red. The spot toward the lower left is one of Jupiter's largest moons: Europa. Images from Voyager in 1979 bolster the modern hypothesis that Europa has an underground ocean and is therefore a good place to look for extraterrestrial life. But what about the dark spot on the upper right? That is a shadow of another of Jupiter's large moons: Io. Voyager 1 discovered Io to be so volcanic that no impact craters could be found. Sixteen frames from Voyager 1's flyby of Jupiter in 1979 were recently reprocessed and merged to create the featured image. Forty-five years ago this September, Voyager 1 launched from Earth and started one of the greatest explorations of the Solar System ever. Free Download: Voyager Posters",https://apod.nasa.gov/apod/image/2207/EuropaJupiter_Voyager_2792.jpg,image,v1,Europa and Jupiter from Voyager 1,https://apod.nasa.gov/apod/image/2207/EuropaJupiter_Voyager_960.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2002-01-02,"High above a cloudy Earth, the International Space Station (ISS) orbits silently. The Space Shuttle Endeavor Crew took the above picture as they departed the space station in mid-December. Endeavor brought up three new astronauts to occupy the ISS and carried home the members of Expedition Three, a trio that has been housed in the ISS since August. Highlights of this Endeavor mission included fixing a solar panel and maneuvering the station to avoid a large piece of passing space junk. Visible in the above picture are the space station's robot manipulator arm as well as several modules and solar arrays.",https://apod.nasa.gov/apod/image/0201/iss_sts108_big.jpg,image,v1,International Space Station Over Earth,https://apod.nasa.gov/apod/image/0201/iss_sts108.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -1997-09-15,"The largest volcano in the Solar System is on Mars. Olympus Mons rises 24 kilometers high and measures 550 km across. By comparison, Earth's largest volcano, Mauna Loa in Hawaii, rises 9 km high and measures 120 km across. Such large volcanoes can exist on Mars because of the low gravity and lack of surface tectonic motion. Olympus Mons is a shield volcano, built by fluid lava. Over the next three years, Mars Global Surveyor, which arrived at Mars last week, will photograph the planet at such high resolution that objects only 100 meters across will be visible. The above image was taken by Mariner 9, which orbited and photographed Mars during 1971 and 1972.",https://apod.nasa.gov/apod/image/9709/mons2_jpl.gif,image,v1,Olympus Mons on Mars: The Largest Volcano,https://apod.nasa.gov/apod/image/9709/mons2_jpl_big.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2023-03-16,"Globular star cluster Omega Centauri, also known as NGC 5139, is 15,000 light-years away. The cluster is packed with about 10 million stars much older than the Sun within a volume about 150 light-years in diameter. It's the largest and brightest of 200 or so known globular clusters that roam the halo of our Milky Way galaxy. Though most star clusters consist of stars with the same age and composition, the enigmatic Omega Cen exhibits the presence of different stellar populations with a spread of ages and chemical abundances. In fact, Omega Cen may be the remnant core of a small galaxy merging with the Milky Way. Omega Centauri's red giant stars (with a yellowish hue) are easy to pick out in this sharp, color telescopic view.",https://apod.nasa.gov/apod/image/2303/NGC5139_Omega_Centauri_3700px.jpg,image,v1,Millions of Stars in Omega Centauri,https://apod.nasa.gov/apod/image/2303/NGC5139_Omega_Centauri_1024px.jpg,Neil Corke,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2002-08-11,"The ongoing Perseid Meteor Shower should be at its strongest on August 12 and 13. The best time to watch will be between 2:00 AM and dawn on Monday morning (so plan on setting your alarm tonight!) and then again on Tuesday. In dark, moonless, predawn skies you may see dozens of meteors per hour. Grains of cosmic sand and gravel shed from Comet Swift-Tuttle will streak across the sky as they vaporize during entry into Earth's atmosphere. Tracing the meteor trails backwards, experienced skygazers will find they converge on the constellation Perseus, thus this annual meteor shower's name. Pictured above is a Perseid meteor from 1993. The colors are representative but digitally enhanced. As the meteor streaked across the night sky, different excited atoms emitted different colors of light. The origin of the green tinge visible at the right is currently unknown, however, and might result from oxygen in Earth's atmosphere.",https://apod.nasa.gov/apod/image/0208/perseid3_sk_big.jpg,image,v1,A Perseid Meteor,https://apod.nasa.gov/apod/image/0208/perseid3_sk.jpg," -S. Kohle & B. Koch, -Bonn University -",exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2024-05-15,"What did the monster active region that created the recent auroras look like when at the Sun's edge? There, AR 3664 better showed its 3D structure. Pictured, a large multi-pronged solar prominence was captured extending from chaotic sunspot region AR 3664 out into space, just one example of the particle clouds ejected from this violent solar region. The Earth could easily fit under this long-extended prominence. The featured image was captured two days ago from this constantly changing region. Yesterday, the strongest solar flare in years was expelled (not shown), a blast classified in the upper X-class. Ultraviolet light from that flare quickly hit the Earth's atmosphere and caused shortwave radio blackouts across both North and South America. Although now rotated to be facing slightly away from the Earth, particles from AR 3664 and subsequent coronal mass ejections (CMEs) might still follow curved magnetic field lines across the inner Solar System and create more Earthly auroras. Gallery: Earth Aurora from Solar Active Region 3664",https://apod.nasa.gov/apod/image/2405/AR3664Prom_Voltmer_1728.jpg,image,v1,AR 3664 at the Sun's Edge,https://apod.nasa.gov/apod/image/2405/AR3664Prom_Voltmer_960.jpg," -Sebastian Voltmer -",exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2005-12-29,"Like delicate cosmic petals, these clouds of interstellar dust and gas have blossomed 1,300 light-years away in the fertile star fields of the constellation Cepheus. Sometimes called the Iris Nebula and dutifully cataloged as NGC 7023, this is not the only nebula in the sky to evoke the imagery of flowers. Still, this beautiful digital image shows off the Iris Nebula's range of colors and symmetries in impressive detail. Within the Iris, dusty nebular material surrounds a massive, hot, young star in its formative years. Central filaments of cosmic dust glow with a reddish photoluminescence as some dust grains effectively convert the star's invisible ultraviolet radiation to visible red light. Yet the dominant color of the nebula is blue, characteristic of dust grains reflecting starlight. Dark, obscuring clouds of dust and cold molecular gas are also present and can lead the eye to see other convoluted and fantastic shapes. Infrared observations indicate that this nebula may contain complex carbon molecules known as PAHs. As shown here, the Iris Nebula is about 6 light-years across.",https://apod.nasa.gov/apod/image/0601/iris_cfht_big.jpg,image,v1,The Iris Nebula from CFHT,https://apod.nasa.gov/apod/image/0601/iris_cfht.jpg,Jean-Charles Cuillandre,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2012-12-24,"Recognized since antiquity and depicted on the shield of Achilles according to Homer, stars of the Hyades cluster form the head of the constellation Taurus the Bull. Their general V-shape is anchored by Aldebaran, the eye of the Bull and by far the constellation's brightest star. Yellowish in appearance, red giant Aldebaran is not a Hyades cluster member, though. Modern astronomy puts the Hyades cluster 151 light-years away making it the nearest established open star cluster, while Aldebaran lies at less than half that distance, along the same line-of-sight. Along with colorful Hyades stars, this stellar holiday portrait locates Aldebaran just below center, as well as another open star cluster in Taurus, NGC 1647 at the left, some 2,000 light-years or more in the background. Just slide your cursor over the image to identify the stars. The central Hyades stars are spread out over about 15 light-years. Formed some 800 million years ago, the Hyades star cluster may share a common origin with M44 (Praesepe), a naked-eye open star cluster in Cancer, based on M44's motion through space and remarkably similar age.",https://apod.nasa.gov/apod/image/1212/HyadesLodriguss.jpg,image,v1,Hyades for the Holidays,https://apod.nasa.gov/apod/image/1212/HyadesLodriguss900.jpg,Catching the Light,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2003-10-29,"Yesterday, our Sun produced one of the most powerful solar flares in recorded history. Seen across the electromagnetic spectrum, the Sun briefly became over 100 times brighter in X-rays than normal. Over the next few days, as energetic particles emitted from these regions strike the Earth, satellite communications might be affected and auroras might develop. The flare and resulting CME, emitted from giant sunspot group 10486, was captured above as it happened by the by the LASCO instrument aboard the Sun-orbiting SOHO satellite. The disk of the Sun is covered to accentuate surrounding areas. The time-lapse movie shows the tremendous explosion in frames separated in real time by about 30 minutes each. The frames appear progressively noisier as protons from the flare begin to strike the detector. The SOHO satellite has been put in a temporary safe mode to avoid damage from the solar particle storm.",https://apod.nasa.gov/apod/image/0310/xflare_soho.gif,image,v1,A Powerful Solar Flare,https://apod.nasa.gov/apod/image/0310/xflare_soho_big.gif,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2021-11-23,"Why are the regions above sunspots so hot? Sunspots themselves are a bit cooler than the surrounding solar surface because the magnetic fields that create them reduce convective heating. It is therefore unusual that regions overhead -- even much higher up in the Sun's corona -- can be hundreds of times hotter. To help find the cause, NASA directed the Earth-orbiting Nuclear Spectroscopic Telescope Array (NuSTAR) satellite to point its very sensitive X-ray telescope at the Sun. Featured here is the Sun in ultraviolet light, shown in a red hue as taken by the orbiting Solar Dynamics Observatory (SDO). Superimposed in false-colored green and blue is emission above sunspots detected by NuSTAR in different bands of high-energy X-rays, highlighting regions of extremely high temperature. Clues about the Sun's atmospheric heating mechanisms come from NuSTAR images like this and shed light on solar nanoflares and microflares as brief bursts of energy that may drive the unusual heating.",https://apod.nasa.gov/apod/image/2111/ActiveSun_NuSTAR_1600.jpg,image,v1,The Sun in X-rays from NuSTAR,https://apod.nasa.gov/apod/image/2111/ActiveSun_NuSTAR_960.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2010-08-10,"Why do some sand dunes on Titan appear backwards? Central Titan, it turns out, is covered by sand, some of which appears strange. Images from the Cassini spacecraft currently orbiting Saturn have uncovered long rows of huge sand dunes near Titan's equator that rise as high as 300 meters. Shadows indicate that most dune shapes are created by wind blowing from the west. The problem is, the typical wind at Titan's equator blows from the east. One recent hypothesis that might solve this grainy conundrum posits that the only winds strong enough to move sand and create dunes occur during rare equinoxes and blow strongly from the west. The above images show a radar swath of Titan's equatorial sand dunes at the top, while similar sand dunes that formed in Namibia on Earth at the bottom. Why central Titan is even covered by so much sand is still being investigated.",https://apod.nasa.gov/apod/image/1008/titanearthdunes_cassini_big.jpg,image,v1,The Sand Dunes of Titan,https://apod.nasa.gov/apod/image/1008/titanearthdunes_cassini.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2020-02-13,"The Trifid Nebula, also known as Messier 20, is easy to find with a small telescope. About 30 light-years across and 5,500 light-years distant it's a popular stop for cosmic tourists in the nebula rich constellation Sagittarius. As its name suggests, visible light pictures show the nebula divided into three parts by dark, obscuring dust lanes. But this penetrating infrared image reveals the Trifid's filaments of glowing dust clouds and newborn stars. The spectacular false-color view is courtesy of the Spitzer Space Telescope. Astronomers have used the infrared image data to count newborn and embryonic stars which otherwise can lie hidden in the natal dust and gas clouds of this intriguing stellar nursery. Launched in 2003, Spitzer explored the infrared Universe from an Earth-trailing solar orbit until its science operations were brought to a close earlier this year, on January 30.",https://apod.nasa.gov/apod/image/2002/trifid_spitzerR.jpg,image,v1,Spitzer's Trifid,https://apod.nasa.gov/apod/image/2002/trifid_spitzerR1024.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2018-10-09,"Many spiral galaxies have bars across their centers. Even our own Milky Way Galaxy is thought to have a modest central bar. Prominently barred spiral galaxy NGC 1672, featured here, was captured in spectacular detail in an image taken by the orbiting Hubble Space Telescope. Visible are dark filamentary dust lanes, young clusters of bright blue stars, red emission nebulas of glowing hydrogen gas, a long bright bar of stars across the center, and a bright active nucleus that likely houses a supermassive black hole. Light takes about 60 million years to reach us from NGC 1672, which spans about 75,000 light years across. NGC 1672, which appears toward the constellation of the Dolphinfish (Dorado), is being studied to find out how a spiral bar contributes to star formation in a galaxy's central regions.",https://apod.nasa.gov/apod/image/1810/NGC1672_Hubble_3600.jpg,image,v1,NGC 1672: Barred Spiral Galaxy from Hubble,https://apod.nasa.gov/apod/image/1810/NGC1672_Hubble_1080.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2016-04-15,"Innermost planet Mercury and a thin crescent Moon are never found far from the Sun in planet Earth's skies. Taken near dusk on April 8, this colorful evening skyscape shows them both setting toward the western horizon just after the Sun. The broad Tagus River and city lights of Lisbon, Portugal run through the foreground under the serene twilight sky. Near perigee or closest approach to Earth, the Moon's bright, slender crescent represents about 3 percent of the lunar disk in sunlight. Of course as seen from the Moon, a nearly full Earth would light up the lunar night, and that strong perigee earthshine makes the rest of the lunar disk visible in this scene. Bright Mercury stays well above the western horizon at sunset for northern skywatchers in the coming days. The fleeting planet reaches maximum elongation, or angular distance from the Sun, on April 18. But Mercury will swing back toward the Sun and actually cross the solar disk on May 9, the first transit of Mercury since November 8, 2006.",https://apod.nasa.gov/apod/image/1604/EarthshineVsMercury_8168-netClaro.jpg,image,v1,Mercury and Crescent Moon Set,https://apod.nasa.gov/apod/image/1604/EarthshineVsMercury_8168-netClaro1048.jpg,Miguel Claro,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2012-05-05,"Rising as the Sun sets, tonight's Full Moon could be hard to miss. Remarkably, its exact full phase (May 6 03:36 UT) will occur less than two minutes after it reaches perigee, the closest point to Earth in the Moon's orbit, making it the largest Full Moon of 2012. The Full Perigee Moon will appear to be some 14 percent larger and 30 percent brighter than a Full Moon near apogee, the most distant point in the elliptical lunar orbit. In comparison, though, it will appear less than 1 percent larger and almost as bright as April's Full Moon, captured in this telephoto image rising over suburban Fort Collins, Colorado, USA. For that lunation, Full Moon and perigee were about 21 hours apart. Of course, if you manage to miss May's Full Perigee Moon, make a note on your calendar. Your next chance to see a Full Moon close to perigee, will be next year on June 23.",https://apod.nasa.gov/apod/image/1205/FullMoonriseArn1250.jpg,image,v1,Full Moonrise,https://apod.nasa.gov/apod/image/1205/FullMoonriseArn600.jpg,Robert Arn,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2024-03-08,"The Tarantula Nebula, also known as 30 Doradus, is more than a thousand light-years in diameter, a giant star forming region within nearby satellite galaxy the Large Magellanic Cloud. About 180 thousand light-years away, it's the largest, most violent star forming region known in the whole Local Group of galaxies. The cosmic arachnid sprawls across this magnificent view, an assembly of image data from large space- and ground-based telescopes. Within the Tarantula (NGC 2070), intense radiation, stellar winds, and supernova shocks from the central young cluster of massive stars cataloged as R136 energize the nebular glow and shape the spidery filaments. Around the Tarantula are other star forming regions with young star clusters, filaments, and blown-out bubble-shaped clouds. In fact, the frame includes the site of the closest supernova in modern times, SN 1987A, at lower right. The rich field of view spans about 2 degrees or 4 full moons in the southern constellation Dorado. But were the Tarantula Nebula closer, say 1,500 light-years distant like the Milky Way's own star forming Orion Nebula, it would take up half the sky.",https://apod.nasa.gov/apod/image/2403/Tarantula-HST-ESO-Webb-LL.jpg,image,v1,The Tarantula Zone,https://apod.nasa.gov/apod/image/2403/Tarantula-HST-ESO-Webb-SS1024.jpg,Robert Gendler,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2020-01-22,"It is the closest cluster of stars to the Sun. The Hyades open cluster is bright enough to have been remarked on even thousands of years ago, yet is not as bright or compact as the nearby Pleiades (M45) star cluster. Pictured here is a particularly deep image of the Hyades which has brings out vivid star colors and faint coincidental nebulas. The brightest star in the field is yellow Aldebaran, the eye of the bull toward the constellation of Taurus. Aldebaran, at 65 light-years away, is now known to be unrelated to the Hyades cluster, which lies about 150 light-years away. The central Hyades stars are spread out over about 15 light-years. Formed about 625 million years ago, the Hyades likely shares a common origin with the Beehive cluster (M44), a naked-eye open star cluster toward the constellation of Cancer, based on M44's motion through space and remarkably similar age.",https://apod.nasa.gov/apod/image/2001/Hyades_Mtanous_1998.jpg,image,v1,The Hyades Star Cluster,https://apod.nasa.gov/apod/image/2001/Hyades_Mtanous_1080.jpg," -Jose Mtanous -",exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2011-04-30,"Tycho! Tycho! burning bright In the darkness of the night, What exploding white dwarf star Did frame thy remnant from afar, In the distant deep dark skies Under gaze of human eyes? Seen by mortals and their ma Named for one called Tycho Brahe.",https://apod.nasa.gov/apod/image/1104/tychosnr_chandra2000c.jpg,image,v1,Tycho's Supernova Remnant,https://apod.nasa.gov/apod/image/1104/tychosnr_chandra900c.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2006-03-11,"Comet Pojmanski flew by planet Earth last weekend on a surprise trip through the inner solar system. Then an easy binocular target for morning skygazers, Pojmanski ultimately showed off a long tail, but it also presented some lovely green-blue hues as gas molecules in its tenuous coma and tail fluoresced in the sunlight. Astronomers Adam Block and Jay GaBany recorded this colorful high-resolution view on March 3rd in the darkness just before twilight. The picture spans about one full moon on the sky. Comet Pojmanski (C/2006 A1) is outward bound and fading now, still visible in binoculars for northern hemisphere observers.",https://apod.nasa.gov/apod/image/0603/c2006a1_blockGabany_f.jpg,image,v1,Colors of Comet Pojmanski,https://apod.nasa.gov/apod/image/0603/c2006a1_blockGabany_c53.jpg," +2021-11-07,"To some it looks like a cat's eye. To others, perhaps like a giant cosmic conch shell. It is actually one of brightest and most highly detailed planetary nebula known, composed of gas expelled in the brief yet glorious phase near the end of life of a Sun-like star. This nebula's dying central star may have produced the outer circular concentric shells by shrugging off outer layers in a series of regular convulsions. The formation of the beautiful, complex-yet-symmetric inner structures, however, is not well understood. The featured image is a composite of a digitally sharpened Hubble Space Telescope image with X-ray light captured by the orbiting Chandra Observatory. The exquisite floating space statue spans over half a light-year across. Of course, gazing into this Cat's Eye, humanity may well be seeing the fate of our sun, destined to enter its own planetary nebula phase of evolution ... in about 5 billion years. APOD in world languages: Arabic, Bulgarian, Catalan, Chinese (Beijing), Chinese (Taiwan), Croatian, Czech, Dutch, French, French (Canada), German, Hebrew, Indonesian, Japanese, Korean, Montenegrin, Polish, Russian, Serbian, Slovenian, Spanish, Taiwanese, Turkish, Turkish, and Ukrainian",https://apod.nasa.gov/apod/image/2111/CatsEye_HubblePohl_1278.jpg,image,v1,The Cat's Eye Nebula in Optical and X-ray,https://apod.nasa.gov/apod/image/2111/CatsEye_HubblePohl_960.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +2014-10-08,"Star cluster NGC 6823 is slowly turning gas clouds into stars. The center of the open cluster, visible on the upper right, formed only about two million years ago and is dominated in brightness by a host of bright young blue stars. Some outer parts of the cluster, visible in the featured image's center as the stars and pillars of emission nebula NGC 6820, contain even younger stars. The huge pillars of gas and dust likely get their elongated shape by erosion from hot radiation emitted from the brightest cluster stars. Striking dark globules of gas and dust are also visible across the upper left of the featured image. Open star cluster NGC 6823 spans about 50 light years and lies about 6000 light years away toward the constellation of the Fox (Vulpecula). APOD Wall Calendar: Nebulas and Star Clusters",https://apod.nasa.gov/apod/image/1410/ngc6823_waid_1092.jpg,image,v1,NGC 6823: Cloud Sculpting Star Cluster,https://apod.nasa.gov/apod/image/1410/ngc6823_waid_1080.jpg," +Donald P. Waid +(Waid Observatory) +",exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +2020-04-15,"It was an astronomical triple play. Setting on the left, just after sunset near the end of last month, was our Moon -- showing a bright crescent phase. Setting on the right was Venus, the brightest planet in the evening sky last month -- and this month, too. With a small telescope, you could tell that Venus' phase was half, meaning that only half of the planet, as visible from Earth, was exposed to direct sunlight and brightly lit. High above and much further in the distance was the Pleiades star cluster. Although the Moon and Venus move with respect to the background stars, the Pleiades do not -- because they are background stars. In the beginning of this month, Venus appeared to move right in front of the Pleiades, a rare event that happens only once every eight years. The featured image captured this cosmic triangle with a series of exposures taken from the same camera over 70 minutes near Avonlea, Saskatchewan, Canada. The positions of the celestial objects was predicted. The only thing unpredicted was the existence of the foreground tree -- and the astrophotographer is still unsure what type of tree that is.",https://apod.nasa.gov/apod/image/2004/MVP_Aspinall_2048.jpg,image,v1,A Cosmic Triangle,https://apod.nasa.gov/apod/image/2004/MVP_Aspinall_960.jpg," +Scott +Aspinall +",exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +2024-03-04,"What's happening across that field? Pictured here are not auroras but nearby light pillars, a phenomenon typically much closer. In most places on Earth, a lucky viewer can see a Sun pillar, a column of light appearing to extend up from the Sun caused by flat fluttering ice-crystals reflecting sunlight from the upper atmosphere. Usually, these ice crystals evaporate before reaching the ground. During freezing temperatures, however, flat fluttering ice crystals may form near the ground in a form of light snow sometimes known as a crystal fog. These ice crystals may then reflect ground lights in columns not unlike a Sun pillar. The featured image was taken last month across the Wulan Butong Grasslands in Inner Mongolia, China.",https://apod.nasa.gov/apod/image/2403/PillarsMongolia_Liao_6240.jpg,image,v1,Light Pillars Over Inner Mongolia,https://apod.nasa.gov/apod/image/2403/PillarsMongolia_Liao_960.jpg," +N. D. Liao +",exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +2016-05-08,"What's that dot on the Sun? If you look closely, it is almost perfectly round. The dot is the result of an unusual type of solar eclipse that occurred in 2006. Usually it is the Earth's Moon that eclipses the Sun. This time, the planet Mercury took a turn. Like the approach to New Moon before a solar eclipse, the phase of Mercury became a continually thinner crescent as the planet progressed toward an alignment with the Sun. Eventually the phase of Mercury dropped to zero and the dark spot of Mercury crossed our parent star. The situation could technically be labeled a Mercurian annular eclipse with an extraordinarily large ring of fire. From above the cratered planes of the night side of Mercury, the Earth appeared in its fullest phase. Hours later, as Mercury continued in its orbit, a slight crescent phase appeared again. This was ten years ago -- the next Mercurian solar eclipse will occur tomorrow. NASA Coverage: Tomorrow's Transit of Mercury across the Sun",https://apod.nasa.gov/apod/image/1605/MercuryTransit_Cortner_1200.jpg,image,v1,Mercury's Transit: An Unusual Spot on the Sun,https://apod.nasa.gov/apod/image/1605/MercuryTransit_Cortner_960.jpg," +David Cortner +",exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +2005-08-31,"What could cause such rays of dark? Dark sky rays were caught in spectacular fashion earlier this month above Utah, USA. The cause is something surprisingly familiar: shadows. Clouds near the horizon can block sunlight from reflecting off air, making columns outward from the Sun appear unusually dark. Cloud shadows can be thought of as the complement of the more commonly highlighted crepuscular rays, also visible above, where sunlight pours though cloud holes. Sometimes, on the opposite side of the sky, anticrepuscular rays can also be seen.",https://apod.nasa.gov/apod/image/0508/sunrise_nesheim_big.jpg,image,v1,Crepuscular Rays Over Utah,https://apod.nasa.gov/apod/image/0508/sunrise_nesheim.jpg," +Jean Nesheim +",exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +2009-04-13,"Just fix your camera to a tripod and you too can make an image of graceful trails traced by the stars as planet Earth rotates on its axis. Making a time lapse video like that shown above may require more effort, though. Made on 2006 October 13 from Mauna Kea, Hawaii, USA, this video nicely captured what you might see of the night sky if you could keep your brain from changing your perceived visual image about every hundredth of a second. Starting from a dark sky and point-like stars, the video demonstrates how stars appear to move over the night as the world turns. Near the center of the developing bull's-eye pattern is Polaris, the North Star. Visible in the left foreground is the 3.7-meter aperture Canada-France-Hawaii Telescope (CFHT). The red glow that illuminated the CFHT dome near the beginning of the film was created by a car leaving the volcanic summit. The Moon rose about half way through the video and created a white glow that gradually illuminated most of the CFHT dome. The above remarkable time-lapse video was constructed from about 1,000 consecutive frames taken with a digital camera over nearly nine hours.",,other,v1,Star Trails over the Canada-France-Hawaii Telescope,,Jean-Charles Cuillandre,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +2005-03-18,"Low on the western horizon after sunset, a slender crescent Moon and wandering planet Mercury join the lights of Menton and Monaco along the French Riviera. Astronomer Vincent Jacques took advantage of this gorgeous photo opportunity a week ago on March 11, when the Moon and Mercury were separated in the sky by just three degrees. Of course, the Moon in a slender crescent phase is always seen near the horizon, as is Mercury - a bright planet which can be otherwise difficult to glimpse as it never strays far from the Sun in Earth's sky. In the coming days good views of Mercury will indeed be fleeting as the solar system's innermost planet is rapidly dropping closer to the glare of the setting Sun. But tonight a waxing Moon will join another bright planet wandering overhead through the evening sky, Saturn.",https://apod.nasa.gov/apod/image/0503/MoonMercMonaco_jacques_full.jpg,image,v1,"Moon, Mercury, Monaco",https://apod.nasa.gov/apod/image/0503/MoonMercMonaco_jacques_f42.jpg," +Vincent Jacques +",exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +2000-08-10,"After the latest round of discovery announcements, the list of known worlds of distant suns has grown to 50. While extrasolar planet discoveries are sure to continue, none - so far - points clearly to another planetary system like our own. Take, for example, the newly discovered parent star HD38529. Shining in Earth's night sky at 6th magnitude, this sun-like star lies 137 light-years away in the constellation Orion. Like most of the known extrasolar planets, HD38529's planet was discovered by detecting the telltale Doppler wobble in the parent star's spectrum. The data reveal that this planet orbits once every 14.3 days at an average of only 0.13 times the Earth-Sun distance and has a minimum of 0.77 Jupiter masses (about 240 Earth masses). There is even evidence in the wobble data that HD38529, and other stars with one known planet have additional massive planets orbiting them. In this dramatic artist's vision, HD38529 and its newfound world are viewed from the moon of another massive ringed planet orbiting farther out. The ringed planet's moon is imagined to have a thin atmosphere and a surface covered with icy sheets and ridges similar to those found on Jupiter's moon Europa.",https://apod.nasa.gov/apod/image/0008/hd38529art_cook.jpg,image,v1,Other Worlds and HD 38529,https://apod.nasa.gov/apod/image/0008/hd38529art_cook.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +2023-11-14,"In the fading darkness before dawn, a tilted triangle appeared to balance atop a rock formation off the southern tip of Sicily. Making up the points of the triangle are three of the four brightest objects visible in Earth’s sky: Jupiter, Venus and the Moon. Though a thin waning crescent, most of the moon’s disk is visible due to earthshine. Captured in this image on 2022 April 27, Venus (center) and Jupiter (left) are roughly three degrees apart -- and were headed toward a close conjunction. Conjunctions of Venus and Jupiter occur about once a year and are visible either in the east before sunrise or in the west after sunset. The featured image was taken about an hour before the arrival of the brightest object in Earth’s sky – the Sun.",https://apod.nasa.gov/apod/image/2311/MoonVenusJupiter_Passalacqua_960.jpg,image,v1,Three Planets Rock,https://apod.nasa.gov/apod/image/2311/MoonVenusJupiter_Passalacqua_960.jpg," +Giovanni Passalacqua; +Text: +Liz Coelho +(Pikes Peak) +",exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +2009-08-11,"What happens when a meteor hits the ground? Usually nothing much, as most meteors are small, and indentations they make are soon eroded away. About 50,000 years ago, however, a large meteor created Barringer Meteor Crater in Arizona, USA. Also known simply as Meteor Crater, the resulting impact basin spans over a kilometer. Pictured above, a tour group views the inside of Barringer Crater early last year. Historically, Barringer Crater was the first feature on Earth to be recognized as an impact crater. Today, over 100 terrestrial impact features have been identified on planet Earth. Computer modeling indicates that some of the Canyon Diablo impactor melted during the impact that created Barringer.",https://apod.nasa.gov/apod/image/0908/barringer_rowell_big.jpg,image,v1,Inside Barringer Meteor Crater,https://apod.nasa.gov/apod/image/0908/barringer_rowell.jpg," +Tony Rowell +",exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +2006-08-12,"Inaugurating the era of space exploration for the US, the First Explorer, a thirty pound satellite, was launched into Earth orbit on January 31, 1958 by the Army Ballistic Missile Agency. Explorer I carried instruments to measure temperatures, micrometeorite impacts, and an experiment designed by James A. Van Allen to measure the density of electrons and ions in space. The measurements made by Van Allen's experiment led to an unexpected and startling discovery -- an earth-encircling belt of high energy electrons and ions trapped in the magnetosphere now known as the Van Allen Radiation Belt. Explorer I ceased transmitting on February 28 of that year but remained in orbit until March of 1970. Pioneering astrophysicist James Van Allen died on August 9th at the age of 91.",https://apod.nasa.gov/apod/image/0608/exp1Launch_msfc_f.jpg,image,v1,The First Explorer,https://apod.nasa.gov/apod/image/0608/exp1Launch_msfc_c22.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +2006-12-14,"Peering through the thick, hazy atmosphere of Saturn's largest moon, an infrared camera onboard the Cassini spacecraft recorded this view of the tallest mountains ever seen on Titan. Captured during a flyby in late October, the high resolution, false-color mosaic shows a mountain range about 150 kilometers long and about 1.5 kilometers high - likened to the Sierra Nevada mountain range of the western United States, planet Earth. Along Titan's mountain ridges lie bright deposits, thought to be methane snow or other organic material. The icy mountains of Titan were probably formed like Earth's mid-ocean ridges, from material welling up to fill gaps created as surface tectonic plates spread apart.",https://apod.nasa.gov/apod/image/0612/PIA09032_titan_mountains.jpg,image,v1,Mountains of Titan,https://apod.nasa.gov/apod/image/0612/PIA09032_titan_mountains720.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +2006-05-12,"Moving rapidly through planet Earth's night sky, Fragment C of crumbling comet 73P/Schwassmann-Wachmann 3 passed almost directly in front of M57 - the Ring Nebula, and faint spiral galaxy IC 1296 on May 8. In fact, in this gorgeous view, the bright head of Fragment C is separated by only about 0.1 degrees from M57, with the tail apparently engulfing nebula and galaxy. Recorded from Elizabeth, Illinois, USA, this picture corresponds to the cosmic scene only 30 minutes after yesterday's picture of the approaching alignment. The relative motion of the comet against the background stars and nebulae is easy to see when comparing the two images. This comet's fragments will be near their closest approach in the coming days, about 10 million kilometers away, and none pose any danger to our fair planet.",https://apod.nasa.gov/apod/image/0605/c73pM57_walker_f.jpg,image,v1,Comet Meets Ring Nebula: Part II,https://apod.nasa.gov/apod/image/0605/c73pM57_walker_c46r.jpg," -Adam Block (Caelum -Observatory), +Sheldon Faworski and Sean Walker +(MASIL +Astro-Imaging Team) -R. Jay GaBany -(Cosmotography.com) +",exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +2004-05-13,"A distinctive X-shape and ladder-like rungs appear in this Hubble Space Telescope image of the intriguing Red Rectangle Nebula. The dusty cosmic cloud was originally identified as a strong source of infrared radiation and is now believed to contain icy dust grains and hydrocarbon molecules formed in the cool outflow from an aging central star. So why does it look like a big X? A likely explanation is that the central star - actually a close pair of stars - is surrounded by a thick dust torus which pinches the otherwise spherical outflow into tip-touching cone shapes. Because we view the torus edge-on, the boundary edges of the cone shapes seem to form an X. The distinct rungs suggest the outflow occurs in fits and starts. About 2,300 light-years away toward the fanciful constellation Monoceros, the Red Rectangle nebula should be transformed into a glorious planetary nebula as its cool central star becomes a hot white dwarf over the next few thousand years. This sharp Hubble picture spans only about one third of a light-year at the distance of the Red Rectangle.",https://apod.nasa.gov/apod/image/0405/redrect_hst_full.jpg,image,v1,Rungs of the Red Rectangle,https://apod.nasa.gov/apod/image/0405/redrect_hst_c1.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +2015-11-25,"Why are there unusual pits on Pluto? The indentations were discovered during the New Horizons spacecraft's flyby of the dwarf planet in July. The largest pits span a kilometer across and dip tens of meters into a lake of frozen nitrogen, a lake that sprawls across Sputnik Planum, part of the famous light-colored heart-shaped region named Tombaugh Regio. Although most pits in the Solar System are created by impact craters, these depressions look different -- many are similarly sized, densely packed, and aligned. Rather, it is thought that something has caused these specific areas of ice to sublimate and evaporate away. In fact, the lack of overlying impact craters indicates these pits formed relatively recently. Even though the robotic New Horizons is now off to a new destination, it continues to beam back to Earth new images and data from its dramatic encounter with Pluto.",https://apod.nasa.gov/apod/image/1511/PlutoPits_NewHorizons_1480.jpg,image,v1,Unusual Pits Discovered on Pluto,https://apod.nasa.gov/apod/image/1511/PlutoPits_NewHorizons_960.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +1999-07-23,Tomorrow's picture: Saturn Day < Archive | Index | Search | Calendar | Glossary | Education | About APOD > Authors & editors: Robert Nemiroff (MTU) & Jerry Bonnell (USRA) NASA Technical Rep.: Jay Norris. Specific rights apply. A service of: LHEA at NASA/ GSFC & Michigan Tech. U.,https://apod.nasa.gov/apod/image/9907/marsvalley_mgs_big.jpg,image,v1,A Martian Valley,https://apod.nasa.gov/apod/image/9907/marsvalley_mgs.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +2003-09-19,"Launched in 1989 and looping through the jovian system since late 1995, the voyage of NASA's Galileo spacecraft will soon come to an end. The spacecraft has been targeted to plunge directly into Jupiter this Sunday, September 21st, at about 30 miles per second. Its components will be vaporized in the gas giant's outer atmosphere. While Galileo's long voyage of exploration has resulted in a spectacular scientific legacy, the spacecraft's ultimate fate is related to perhaps its most tantalizing discovery -- strong evidence for a liquid ocean beneath the frozen surface of Jupiter's moon Europa. Galileo is now almost completely out of fuel for maneuvers, so this intentional collision with Jupiter will prevent any unintentional future collision with Europa and the possibility of contaminating the jovian moon with microbes from Earth hardy enough to survive in interplanetary space. Color image data from the Galileo mission recorded between 1995 and 1998 was used to create this depiction of Europa's cracked and icy surface. The inset shows dark reddish, disrupted regions dubbed Thera and Thrace.",https://apod.nasa.gov/apod/image/0309/europa1_gal_full.jpg,image,v1,Galileo's Europa,https://apod.nasa.gov/apod/image/0309/europa1_gal_c1.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +1997-11-24,"stein's Special Theory of Relativity says that nothing can travel faster than the speed of light. Jets of protons and electrons that shoot away from objects such as quasars and black holes appear to travel at speeds approaching this maximum speed, though. Such jets carry tremendous energy and can ram straight through interstellar material. In the above frame from a computer simulation, a jet traveling only 98 percent of light speed rams and mixes with interstellar material. Even higher energy jets might well explain the structure seen around Cygnus A.",https://apod.nasa.gov/apod/image/9711/cygjet2_umi_big.gif,image,v1,Jet Near Light Speed,https://apod.nasa.gov/apod/image/9711/cygjet2_umi.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +2014-01-04,"A crescent Venus shines along the western horizon at dusk in this clearing sky. The Earth's sister planet is smiling between the low clouds near the bottom of the frame during its January 2nd conjunction with the slender, young crescent Moon above. Of course the lovely pairing of Moon and Venus crescents could be enjoyed in the new year's skies around the the world. But the twin contrails in this scene belong to an aircraft above Appenzell, Switzerland. Soon to disappear from evening skies, Venus is heading toward its January 11th inferior conjunction and an appearance in predawn skies as planet Earth's morning star by late January. And the Moon will be young again, too.",https://apod.nasa.gov/apod/image/1401/Crescents2014_CMalinDSC8382s.jpg,image,v1,Clouds and Crescents,https://apod.nasa.gov/apod/image/1401/Crescents2014_CMalinDSC8382s.jpg,Christoph Malin,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +2023-09-01,"In 1716, English astronomer Edmond Halley noted, ""This is but a little Patch, but it shows itself to the naked Eye, when the Sky is serene and the Moon absent."" Of course, M13 is now less modestly recognized as the Great Globular Cluster in Hercules, one of the brightest globular star clusters in the northern sky. Sharp telescopic views like this one reveal the spectacular cluster's hundreds of thousands of stars. At a distance of 25,000 light-years, the cluster stars crowd into a region 150 light-years in diameter. Approaching the cluster core, upwards of 100 stars could be contained in a cube just 3 light-years on a side. For comparison, the closest star to the Sun is over 4 light-years away. The remarkable range of brightness recorded in this image follows stars into the dense cluster core.",https://apod.nasa.gov/apod/image/2309/M13-totale-en-cours-crop8.jpg,image,v1,The Great Globular Cluster in Hercules,https://apod.nasa.gov/apod/image/2309/M13-totale-en-cours-crop8_1024.jpg,"Serge Brunier, Jean-François Bax, David Vernet",exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +2010-09-14,"What created the strange spiral structure on the left? No one is sure, although it is likely related to a star in a binary star system entering the planetary nebula phase, when its outer atmosphere is ejected. The huge spiral spans about a third of a light year across and, winding four or five complete turns, has a regularity that is without precedent. Given the expansion rate of the spiral gas, a new layer must appear about every 800 years, a close match to the time it takes for the two stars to orbit each other. The star system that created it is most commonly known as LL Pegasi, but also AFGL 3068. The unusual structure itself has been cataloged as IRAS 23166+1655. The above image was taken in near-infrared light by the Hubble Space Telescope. Why the spiral glows is itself a mystery, with a leading hypothesis being illumination by light reflected from nearby stars.",https://apod.nasa.gov/apod/image/1009/llpegspiral_hst_big.jpg,image,v1,An Extraordinary Spiral from LL Pegasi,https://apod.nasa.gov/apod/image/1009/llpegspiral_hst.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +2011-07-12,"Here is one of the largest objects that anyone will ever see on the sky. Each of these fuzzy blobs is a galaxy, together making up the Perseus Cluster, one of the closest clusters of galaxies. The cluster is seen through a foreground of faint stars in our own Milky Way Galaxy. Near the cluster center, roughly 250 million light-years away, is the cluster's dominant galaxy NGC 1275, seen above as a large galaxy on the image left. A prodigious source of x-rays and radio emission, NGC 1275 accretes matter as gas and galaxies fall into it. The Perseus Cluster of Galaxies, also cataloged as Abell 426, is part of the Pisces-Perseus supercluster spanning over 15 degrees and containing over 1,000 galaxies. At the distance of NGC 1275, this view covers about 15 million light-years.",https://apod.nasa.gov/apod/image/1107/abell426_franke_1800.jpg,image,v1,The Perseus Cluster of Galaxies,https://apod.nasa.gov/apod/image/1107/abell426_franke_900.jpg," +Bob Franke +",exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +2000-01-07,"Dazzling displays of star formation abound across the face of galaxy NGC 4214, a mere 13 million light-years away in the northern constellation Canes Venatici. While this 1997 Hubble Space Telescope image shows the numerous faint, older stars of NGC 4214, the most eye-catching features are the galaxy's bright young star clusters surrounded by fluorescent gas clouds. Sculpted into bubbles and filamentary shapes by energetic explosions and stellar winds from massive cluster stars, the clouds fluoresce in the intense stellar ultraviolet radiation. The colorful spectacle of massive young star forming clusters and distinguished presence of a fainter, older stellar population indicate that NGC 4214 has experienced star formation episodes spanning billions of years.",https://apod.nasa.gov/apod/image/0001/ngc4214_hst_big.jpg,image,v1,NGC 4214: Star Forming Galaxy,https://apod.nasa.gov/apod/image/0001/ngc4214_hst.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +2003-09-01,"The beautiful Trifid Nebula (aka M20), a photogenic study in cosmic contrasts, lies about 5,000 light-years away toward the nebula rich constellation Sagittarius. A star forming region in the plane of our galaxy, the Trifid alone illustrates three basic types of astronomical nebulae; red emission nebulae dominated by light from hydrogen atoms, blue reflection nebulae produced by dust reflecting starlight, and dark absorption nebulae where dense dust clouds appear in silhouette. The bright emission nebula on the right, separated into three parts by obscuring dust lanes, lends the nebula its popular name. Many details are apparent in this gorgeous high-resolution image of the Trifid. For example, light-year long pillars and jets sculpted by newborn stars - visible here in the upper right-hand corner of the emission nebula - appear in Hubble Space Telescope close-up images of the region.",https://apod.nasa.gov/apod/image/0308/m20castano_block_full.jpg,image,v1,A Beautiful Trifid,https://apod.nasa.gov/apod/image/0308/m20castano_block_c1.jpg," -",exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2022-12-18,"Do you know the names of some of the brightest stars? It's likely that you do, even though some bright stars have names so old they date back to near the beginning of written language. Many world cultures have their own names for the brightest stars, and it is culturally and historically important to remember them. In the interest of clear global communication, however, the International Astronomical Union (IAU) has begun to designate standardized star names. Featured here in true color are the 25 brightest stars in the night sky, currently as seen by humans, coupled with their IAU-recognized names. Some star names have interesting meanings, including Sirius (""the scorcher"" in Latin), Vega (""falling"" in Arabic), and Antares (""rival to Mars"" in Greek). You are likely even familiar with the name of at least one star too dim to make this list: Polaris. Almost Hyperspace: Random APOD Generator",https://apod.nasa.gov/apod/image/2212/25BrightestStars_Jittasaiyapan_1500.jpg,image,v1,25 Brightest Stars in the Night Sky,https://apod.nasa.gov/apod/image/2212/25BrightestStars_Jittasaiyapan_960.jpg," -Tragoolchitr Jittasaiyapan -",exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2021-09-27,"Here is one of the most famous pictures from the Moon -- but digitally reversed. Apollo 11 landed on the moon in 1969 and soon thereafter many pictures were taken, including an iconic picture of Buzz Aldrin taken by Neil Armstrong. The original image captured not only the magnificent desolation of an unfamiliar world, but Armstrong himself reflected in Aldrin's curved visor. Enter modern digital technology. In the featured image, the spherical distortion from Aldrin's helmet has been reversed. The result is the famous picture -- but now featuring Armstrong himself from Aldrin's perspective. Even so, since Armstrong took the picture, the image is effectively a five-decade old lunar selfie. The original visor reflection is shown on the left, while Earth hangs in the lunar sky on the upper right. A foil-wrapped leg of the Eagle lander is prominently visible. Preparations to return humans to the Moon in the next few years include the Artemis program, an international collaboration led by NASA.",https://apod.nasa.gov/apod/image/2109/AldrinVisor_Apollo11_4096.jpg,image,v1,Unwrapped: Five Decade Old Lunar Selfie,https://apod.nasa.gov/apod/image/2109/AldrinVisorCrop_Apollo11_1080.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2011-11-29,"A fantastic jumble of young blue star clusters, gigantic glowing gas clouds, and imposing dark dust lanes surrounds the central region of the active galaxy Centaurus A. This image from the Hubble Space Telescope has been processed to present a natural color picture of this cosmic maelstrom. Infrared images from the Hubble have also shown that hidden at the center of this activity are what seem to be disks of matter spiraling into a black hole with a billion times the mass of the Sun. Centaurus A itself is apparently the result of a collision of two galaxies and the left over debris is steadily being consumed by the black hole. Astronomers believe that such black hole central engines generate the radio, X-ray, and gamma-ray energy radiated by Centaurus A and other active galaxies. But for an active galaxy Centaurus A is close, a mere 10 million light-years away, and is a relatively convenient laboratory for exploring these powerful sources of energy. APOD Graduate Assistantship: Research the universe - support a leading astronomy web site",https://apod.nasa.gov/apod/image/1111/cenA2_hst_3989.jpg,image,v1,Across the Center of Centaurus A,https://apod.nasa.gov/apod/image/1111/cenA2_hst_900.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2012-05-09,"What's that in the background? Two famous New York City icons stand tall in the above photo taken last week. On the left looms the Statue of Liberty, a universal symbol of freedom, while on the right rises the Empire State Building, now the second largest building in the city. What's unique about this once-in-a-lifetime photograph, though, is the third icon that appears to Lady Liberty's left. High in the air and far in the background flies the space shuttle Enterprise -- perched atop a 747 jet -- on the way to its new home. New Yorkers and visitors to the Big Apple can visit the test space shuttle at the Intrepid Sea, Air & Space Museum on the West Side of Manhattan starting July 19. Neptune & Vulcan Astronomy Seminar of the Week",https://apod.nasa.gov/apod/image/1205/shuttlelibertyempire_nasa_836.jpg,image,v1,Shuttle Enterprise Over New York,https://apod.nasa.gov/apod/image/1205/shuttlelibertyempire_nasa_960.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2014-03-15,"Get out your red/blue glasses and check out this stereo scene from Taurus-Littrow valley on the Moon! The color anaglyph features a detailed 3D view of Apollo 17's Lunar Rover in the foreground -- behind it lies the Lunar Module and distant lunar hills. Because the world was going to be able to watch the Lunar Module's ascent stage liftoff via the rover's TV camera, this parking place was also known as the VIP Site. In December of 1972, Apollo 17 astronauts Eugene Cernan and Harrison Schmitt spent about 75 hours on the Moon, while colleague Ronald Evans orbited overhead. The crew returned with 110 kilograms of rock and soil samples, more than from any of the other lunar landing sites. Cernan and Schmitt are still the last to walk (or drive) on the Moon.",https://apod.nasa.gov/apod/image/1403/a17anaglyph_vanMeijgaarden_f.jpg,image,v1,Apollo 17 VIP Site Anaglyph,https://apod.nasa.gov/apod/image/1403/a17anaglyph_vanMeijgaarden_c800.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2003-01-27,"What is happening to molecular cloud BHR 71? Quite possible, a binary star system is forming inside. Most stars in our Galaxy are part of binary star systems, but few have ever been seen in formation. Recent observations of dust-darkened Bok Globule BHR 71, however, show evidence for two young stars forming deep in the cloud, likely close enough to form a binary. Isolated BHR 71 spans about one light year and lies only about 600 light years away in the southern sky. The brighter embedded star -- not visible here -- is about 10 times as bright as the Sun and drives the jet that swept out the empty lane. The above four-color image was taken with a Very Large Telescope in Chile.",https://apod.nasa.gov/apod/image/0301/bhr71_vlt_big.jpg,image,v1,"BHR 71: Stars, Clouds, and Jets",https://apod.nasa.gov/apod/image/0301/bhr71_vlt.jpg," -J. Alves -(ESO), -E. Tolstoy (Groningen), -R. Fosbury (ST-ECF), & -R. Hook (ST-ECF), -VLT -",exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2010-04-09,"On April 5, visitors to Kennedy Space Center saw these colorful clouds, twisting and drifting through dawn skies. Of course, the clouds were rocket engine plumes from the predawn launch of the space shuttle Discovery on the STS-131 mission to the International Space Station. Their layered colors are created as they reflect the reddened light from the still rising Sun. Fittingly, denizens of the space center's rocket garden are lit in the foreground. At the far left is a 1960s vintage multistage Atlas-Agena rocket. Together on the right, are Mercury-Redstone and Mercury-Atlas rockets.",https://apod.nasa.gov/apod/image/1004/DRocketGard_craigcrawford.jpg,image,v1,Discovery's Dawn,https://apod.nasa.gov/apod/image/1004/DRocketGard_craigcrawford900.jpg,rocket engine plumes,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2006-02-18,"This dream-like image of Mir was recorded by astronauts as the space shuttle orbiter Atlantis approached the Russian space station prior to docking during the STS-76 mission in 1996. Sporting spindly appendages and solar panels, Mir resembles a whimsical flying insect hovering about 350 kilometers above New Zealand's South Island and the city of Nelson near Cook Strait. Mir was launched 20 years ago this week, and served as a continuously occupied orbital outpost until August 1999. Mir was visited by over 100 spacefarers from the nations of planet Earth including, Russia, the United States, Great Britain, Germany, France, Japan, Austria, Kazakhstan and Slovakia. The Mir was deorbited in March 2001.",https://apod.nasa.gov/apod/image/0602/mirdream_sts76_big.jpg,image,v1,Mir Dreams,https://apod.nasa.gov/apod/image/0602/mirdream_sts76.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2001-10-20,"Tune your radio telescope to 408MHz (408 million cycles per second) and check out the Radio Sky! You should find that frequency on your dial somewhere between US broadcast television channels 13 and 14. In the 1970s large dish antennas at three radio observatories, Jodrell Bank, MPIfR, and Parkes Observatory, were used to do just that - the data were combined to map the entire sky. Near this frequency, cosmic radio waves are generated by high energy electrons spiraling along magnetic fields. In the resulting false color image, the galactic plane runs horizontally through the center, but no stars are visible. Instead, many of the bright sources near the plane are distant pulsars, star forming regions, and supernova remnants, while the grand looping structures are pieces of bubbles blown by local stellar activity. External galaxies like Centaurus A, located above the plane to the right of center, and the LMC (below and right) also shine in the Radio Sky.",https://apod.nasa.gov/apod/image/0110/408_allsky_big.gif,image,v1,The Radio Sky: Tuned to 408MHz,https://apod.nasa.gov/apod/image/0110/408_allsky.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2015-03-28,"Near the March 20 equinox the cold clear sky over Longyearbyen, Norway, planet Earth held an engaging sight, a total eclipse of the Sun. The New Moon's silhouette at stages just before and after the three minute long total phase seems to sprout glistening diamonds and bright beads in this time lapse composite of the geocentric celestial event. The last and first glimpses of the solar disk with the lunar limb surrounded by the glow of the Sun's inner corona give the impression of a diamond ring in the sky. At the boundaries of totality, sunlight streaming through valleys in the irregular terrain along the Moon's edge, produces an effect known as Baily's Beads, named after English astronomer Francis Baily who championed an explanation for the phenomenon in 1836. This sharp composition also shows off the array of pinkish solar prominences lofted above the edge of the eclipsed Sun.",https://apod.nasa.gov/apod/image/1503/TSE2015Bailysbeads_WangLetian.jpg,image,v1,Diamond Rings and Baily's Beads,https://apod.nasa.gov/apod/image/1503/TSE2015Bailysbeads_WangLetian1024c.jpg,"Wang, Letian",exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -1996-02-23,"Apollo 15 astronaut James Irwin works on the first Lunar Roving Vehicle, before he and fellow astronaut David Scott take it out for a drive. Sloping up behind the lunar module ""Falcon"" on the left are lunar mountains Hadley Delta and Apennine Front, while about 5 kilometers behind Irwin is St. George Crater. The explorations conducted during the Apollo lunar missions discovered much about our Moon, including that the Moon is made of ancient rock, that the Moon's composition is similar to Earth's, that life is not evident there, that the Moon underwent a great hot melting in its distant past, that the Moon has suffered from numerous impacts as shown by its craters, and that the Moon's surface is covered by a layer of rock fragments and dust.",https://apod.nasa.gov/apod/image/lunrov_a15_big.gif,image,v1,Apollo 15: Driving on the Moon,https://apod.nasa.gov/apod/image/lunrov_a15.gif,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -1996-05-05,"What would the night sky look like if you lived on a planet near the center of a galaxy? Now imagine that this galaxy houses a black hole billions of times more massive than a star. From this spectacular vantage point, the sky might look like the above illustration. This drawing is based on recent observations of the center of NGC 4261, made by the Hubble Space Telescope. Results indicate that a disk of dust 800-light years wide surrounds the black hole. The hypothetical planet depicted above lies within this disk. The black hole itself heats gas to white-hot temperatures, generating light that is reddened when reflected off the dust. Jets shoot off from the poles of the black hole, perpendicular to the disk. However, friction with the dust and gas would cause planets near the black hole to spiral in and disappear forever. NASA has recently announced a new initiative to search for Earth-like planets in our Galaxy.",https://apod.nasa.gov/apod/image/ngc4261_art_jg_big.jpg,image,v1,Planet Near a Galaxy Core,https://apod.nasa.gov/apod/image/ngc4261_art_jg.gif,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2011-12-31,"On December 24, Comet Lovejoy rose in dawn's twilight, arcing above the eastern horizon, its tails swept back by the solar wind and sunlight. Seen on the left is the comet's early morning appearance alongside the southern Milky Way from the town of Intendente Alvear, La Pampa province, Argentina. The short star trails include bright southern sky stars Alpha and Beta Centauri near the center of the frame, but the long bright streak that crosses the comet tails is a little closer to home. Waiting for the proper moment to start his exposure, the photographer has also caught the International Space Station still glinting in the sunlight as it orbits (top to bottom) above the local horizon. The right panel is the near horizon view of Comet Lovejoy from the space station itself, captured only two days earlier. In fact, Dan Burbank, Expedition 30 commander, recorded Comet Lovejoy rising just before the Sun in a spectacular video (linked here). Even considering the other vistas available from low Earth orbit, Burbank describes the comet as ""the most amazing thing I have ever seen in space.""",https://apod.nasa.gov/apod/image/1112/ISSLovejoy2panel.jpg,image,v1,Comet Lovejoy and the ISS,https://apod.nasa.gov/apod/image/1112/ISSLovejoy2panel.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -1998-12-02,"This new deep view of the cosmos is the sequel to the 1995 hit Hubble Space Telescope Deep Field. Billed as the Hubble Deep Field South, it was produced by pointing the space telescope toward a patch of sky in the southern constellation Tucana. Over a period of 10 days, many separate exposures were accumulated and combined to reveal progressively fainter galaxies. The original deep field was constructed by observing a piece of sky in the northern constellation Ursa Major. Both stare down 12 billion light-year long tunnels to far-off and still mysterious times when young galaxies inhabited an infant universe. Hubble Deep Field South observations were released to an enthusiastic audience on November 23, 1998.",https://apod.nasa.gov/apod/image/9812/southerndeep_hst_big.jpg,image,v1,A Deep Field In The Southern Sky,https://apod.nasa.gov/apod/image/9812/southerndeep_hst.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2016-01-03,"On some nights, the sky is the best show in town. On this night, the sky was not only the best show in town, but a composite image of the sky won an international competition for landscape astrophotography. The featured winning image was taken in 2011 over J�kuls�rl�n, the largest glacial lake in Iceland. The photographer combined six exposures to capture not only two green auroral rings, but their reflections off the serene lake. Visible in the distant background sky is the band of our Milky Way Galaxy and the Andromeda galaxy. A powerful coronal mass ejection from the Sun caused auroras to be seen as far south as Wisconsin, USA. Solar activity over the past week has resulted in auroras just over the past few days. Follow APOD on: Facebook, Google Plus, or Twitter",https://apod.nasa.gov/apod/image/1601/aurora_vetter_2000.jpg,image,v1,A Starry Night of Iceland,https://apod.nasa.gov/apod/image/1601/aurora_vetter_1080.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2000-05-26,"Nearly 400 years ago astronomer Johannes Kepler observed comet tails blown by a solar breeze and suggested that vessels might likewise navigate through space using appropriately fashioned sails. It is now widely recognized that sunlight does indeed produce a force which moves comet tails and a large, reflective sail could be a practical means of propelling a spacecraft. In fact, the illustration above represents one concept currently being explored by NASA centers to develop an interstellar probe pushed along by sunlight reflected from an ultrathin sail. Nearly half a kilometer wide, the delicate solar sail would be unfurled in space. Continuous pressure from sunlight would ultimately accelerate the craft to speeds about five times higher than possible with conventional rockets -- without requiring any fuel! If launched in 2010 such a probe could overtake Voyager 1, the most distant spacecraft bound for interstellar space, in 2018 going as far in eight years as the Voyager will have journeyed in 41 years.",https://apod.nasa.gov/apod/image/0005/solarsail_msfc_m.jpg,image,v1,Solar Sail,https://apod.nasa.gov/apod/image/0005/solarsail_msfc.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2015-01-17,"Sweeping north in planet Earth's sky, Comet Lovejoy's greenish coma and blue tinted ion tail stretched across this field of stars in the constellation Taurus on January 13. The inset at the upper left shows the 1/2 degree angular size of the full moon for scale. So Lovejoy's coma appears only a little smaller (but much fainter) than a full moon on the sky, and its tail is visible for over 4 degrees across the frame. That corresponds to over 5 million kilometers at the comet's estimated distance of 75 million kilometers from Earth. Blown by the solar wind, the comet's tenuous, structured ion tail streams away from the Sun, growing as this Comet Lovejoy heads toward perihelion, its closest approach to the Sun, on January 30. While diatomic carbon (C2) gas fluorescing in sunlight produces the coma's green color, the fainter bluish tail is tinted by emission from ionized carbon monoxide (CO+).",https://apod.nasa.gov/apod/image/1501/lovejoyJan13RBA.jpg,image,v1,Comet Lovejoy's Tail,https://apod.nasa.gov/apod/image/1501/lovejoyJan13RBA1024.jpg,"Rogelio Bernal -Andreo",exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2001-01-22,Tomorrow's picture: Big Space Ball < | Archive | Index | Search | Calendar | Glossary | Education | About APOD | > Authors & editors: Robert Nemiroff (MTU) & Jerry Bonnell (USRA) NASA Technical Rep.: Jay Norris. Specific rights apply. A service of: LHEA at NASA/GSFC & Michigan Tech. U.,https://apod.nasa.gov/apod/image/0101/whitecrater_near_big.jpg,image,v1,A Two Toned Crater on Asteroid Eros,https://apod.nasa.gov/apod/image/0101/whitecrater_near.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2003-08-25,"Many of the stars in our home Milky Way Galaxy appear together as a dim band on the sky that passes nearly over the Earth's north and south poles. Pictured above is the part of our Galaxy that passes closest over the north pole. Placing your cursor over the image will bring up the names of several constellations and bright stars. The diffuse white Galaxy glow is created by billions of stars, while red patches are large emission nebulas, usually marking areas where bright stars have recently formed. In the north, all of the lights visible at night and all lights that created this image were emitted within the past few thousand years from within the Milky Way Galaxy -- except one. On the upper right is a small faint patch designated M31, the Andromeda Galaxy. M31 is a spiral galaxy similar to our Milky Way but so distant it emits the oldest light distinguishable by the unaided eye -- light that takes over two million years to reach us.",https://apod.nasa.gov/apod/image/0308/northmilkyway_lodriguss_plain.jpg,image,v1,The Northern Milky Way,https://apod.nasa.gov/apod/image/0308/northmilkyway_lodriguss_plain.jpg,Astropix.com,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2022-03-21,"What if you could see the entire sky -- all at once -- for an entire year? That, very nearly, is what is pictured here. Every 15 minutes during 2021, an all-sky camera took an image of the sky over the Netherlands. Central columns from these images were then aligned and combined to create the featured keogram, with January at the top, December at the bottom, and the middle of the night running vertically just left of center. What do we see? Most obviously, the daytime sky is mostly blue, while the nighttime sky is mostly black. The twelve light bands crossing the night sky are caused by the glow of the Moon. The thinnest part of the black hourglass shape occurs during the summer solstice when days are the longest, while the thickest part occurs at the winter solstice. Yesterday was an equinox -- when night and day were equal -- and the northern-spring equinox from one year ago can actually be located in the keogram -- about three-quarters of the way up. Follow APOD on Instagram in: English, Indonesian, Persian, Portuguese or Taiwanese",https://apod.nasa.gov/apod/image/2203/YearOfSky_Bassa_960.jpg,image,v1,The Sky in 2021,https://apod.nasa.gov/apod/image/2203/YearOfSky_Bassa_960.jpg," -Cees Bassa -(Netherlands Institute for Radio Astronomy) -",exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2013-05-11,"This week the shadow of the New Moon fell on planet Earth, crossing Queensland's Cape York in northern Australia ... for the second time in six months. On the morning of May 10, the Moon's apparent size was too small to completely cover the Sun though, revealing a ""ring of fire"" along the central path of the annular solar eclipse. Near mid-eclipse from Coen, Australia, a webcast team captured this telescopic snapshot of the annular phase. Taken with a hydrogen-alpha filter, the dramatic image finds the Moon's silhouette just within the solar disk, and the limb of the active Sun spiked with solar prominences. Still, after hosting back-to-back solar eclipses, northern Australia will miss the next and final solar eclipse of 2013. This November, a rare hybrid eclipse will track across the North Atlantic and equatorial Africa.",https://apod.nasa.gov/apod/image/1305/ASE_McCarty3-3.jpg,image,v1,Cape York Annular Eclipse,https://apod.nasa.gov/apod/image/1305/ASE_McCarty3-3sc900.jpg,MWV Observatory,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -1995-07-03,"July 3, 1995 The Great Nebula in Orion Picture Credit: NASA, Hubble Space Telescope Explanation: The Great Nebula in Orion, M42, can be found on the night sky just below and to the left of the easily identifiable belt of three stars in the popular constellation Orion. This nebula is one of the closest stellar nurseries - where young stars are being formed even now. Clumps of gas (mostly hydrogen and helium) and dust in the nebula are squeezed together by their own gravity until they collapse and form stars. Some stars we can see here partially obscured by the nebula, are only about 100,000 years old - just babies compared to the 5 billion (5,000,000,000) years of our Sun. For more information see NASA, Hubble Space Telescope Scientific Institute press release. We keep an archive of Astronomy Pictures of the Day. Astronomy Picture of the Day is brought to you by Robert Nemiroff and Jerry Bonnell . Original material on this page is copyrighted to Robert J. Nemiroff and Jerry T. Bonnell.",https://apod.nasa.gov/apod/image/orion_hst.gif,image,v1,The Great Nebula in Orion,https://apod.nasa.gov/apod/image/orion_hst.gif,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -1999-03-24,"The spot near the bottom is an image of an unusual type of object: a brown dwarf. A brown dwarf is sometimes called a ""failed star"" because it does not have enough mass to shine by nuclear fusion. A brown dwarf is more massive than a planet, though, and thought to have formed through stellar-like nebular condensation. Brown dwarfs and planets are likely quite abundant, but usually difficult to see in the glare of brighter stars they orbit. New techniques, such as using coronagraphic masks to block the light of the bright star, are allowing the detection of these faint stellar companions. Above, much of the bright light of central Gliese 229A has been blocked and digitally subtracted, leaving the clearest image yet of Gliese 229B. Perfecting techniques like this increases ability to detect still dimmer Earth-type planets orbiting nearby stars.",https://apod.nasa.gov/apod/image/9903/gl229_irtf.jpg,image,v1,Brown Dwarf Gliese 229B,https://apod.nasa.gov/apod/image/9903/gl229_irtf_big.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2018-12-24,"""Oh my God! Look at that picture over there! Here's the Earth coming up. Wow is that pretty!"" Soon after that pronouncement, 50 years ago today, one of the most famous images ever taken was snapped from the orbit of the Moon. Now known as ""Earthrise"", the iconic image shows the Earth rising above the limb of the Moon, as taken by the crew of Apollo 8. But the well-known Earthrise image was actually the second image taken of the Earth rising above the lunar limb -- it was just the first in color. With modern digital technology, however, the real first Earthrise image -- originally in black and white -- has now been remastered to have the combined resolution and color of the first three images. Behold! The featured image is a close-up of the picture that Apollo 8 astronaut Bill Anders was talking about. Thanks to modern technology and human ingenuity, now we can all see it. (Historical note: A different historic black & white image of the Earth setting behind the lunar limb was taken by the robotic Lunar Orbiter 1 two years earlier.)",https://apod.nasa.gov/apod/image/1812/Earthrise1_Apollo8AndersWeigang_2048.jpg,image,v1,Earthrise 1: Historic Image Remastered,https://apod.nasa.gov/apod/image/1812/Earthrise1_Apollo8AndersWeigang_960.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2022-03-03,"A mere 46 million light-years distant, spiral galaxy NGC 2841 can be found in the northern constellation of Ursa Major. This deep view of the gorgeous island universe was captured during 32 clear nights in November, December 2021 and January 2022. It shows off a striking yellow nucleus, galactic disk, and faint outer regions. Dust lanes, small star-forming regions, and young star clusters are embedded in the patchy, tightly wound spiral arms. In contrast, many other spirals exhibit grand, sweeping arms with large star-forming regions. NGC 2841 has a diameter of over 150,000 light-years, even larger than our own Milky Way. X-ray images suggest that resulting winds and stellar explosions create plumes of hot gas extending into a halo around NGC 2841.",https://apod.nasa.gov/apod/image/2203/NGC2841_20220114_72H.jpg,image,v1,Spiral Galaxy NGC 2841,https://apod.nasa.gov/apod/image/2203/NGC2841_20220114_72H_1024.jpg,Vitali Pelenjow,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2002-06-16,"Why does Jupiter have rings? Jupiter's rings were discovered in 1979 by the passing Voyager 1 spacecraft, but their origin was a mystery. Data from the Galileo spacecraft currently orbiting Jupiter later confirmed that these rings were created by meteoroid impacts on small nearby moons. As a small meteoroid strikes tiny Adrastea, for example, it will bore into the moon, vaporize, and explode dirt and dust off into a Jovian orbit. Pictured above is an eclipse of the Sun by Jupiter, as viewed from Galileo. Small dust particles high in Jupiter's atmosphere, as well as the dust particles that compose the rings, can be seen by reflected sunlight. Anniversary: APOD Turns Seven",https://apod.nasa.gov/apod/image/0206/jupring1_gal_big.jpg,image,v1,Jupiter's Rings Revealed,https://apod.nasa.gov/apod/image/0206/jupring1_gal.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -1998-03-24,"What's the farthest galaxy known? The answer keeps changing as astronomers compete to find new galaxies which top the list. The new record holder is now the faint red smudge indicated in the above image by the arrow. Detected light left this galaxy billions of years ago, well before the Earth formed, when the universe was younger than 1/10th of its present age. Astronomers have measured a redshift of 5.34 for this galaxy, breaking the ""5 barrier"" for the first time. Young galaxies are of much interest to astronomers because many unanswered questions exist on when and how galaxies formed in the early universe. Although this galaxy's distance exceeds that of even the farthest known quasar, it is still in front of the pervasive glowing gas that is now seen as the cosmic microwave background radiation.",https://apod.nasa.gov/apod/image/9803/gal5p34_keck_big.gif,image,v1,A Baby Galaxy,https://apod.nasa.gov/apod/image/9803/gal5p34_keck.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2007-10-24,"Scroll right and cruise above the thin, icy rings of Saturn. This high resolution scan is a mosaic of images presented in natural color and recorded in May, over about 2.5 hours as the Cassini spacecraft passed above the unlit side of the rings. The rings themselves are seen to be composed of many individual ringlets. To help track your progress, the rings are labeled below, along with the distance from the center of the gas giant in kilometers. Major ring gaps are labeled above. The alphabetical designation of Saturn's rings is historical and related to their order of discovery; rings A and B are the bright rings separated by the Cassini division. In order of increasing distance from Saturn, the seven main rings run D,C,B,A,F,G,E. (Faint, outer rings G and E are not imaged here.)",https://apod.nasa.gov/apod/image/0710/PIA08389_fig1.jpg,image,v1,Ring Scan,https://apod.nasa.gov/apod/image/0710/PIA08389_fig1_h500.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -1997-06-22,"This Hubble Space Telescope image of a group of faint galaxies ""far, far away"" is a snap shot of the Universe when it was young. The bluish, irregularly shaped galaxies revealed in the image are up to eight billion light years away and seem to have commonly undergone galaxy collisions and bursts of star formation. Studying these objects is difficult because they are so faint, however they may provide clues to how our own Milky Way Galaxy formed.",https://apod.nasa.gov/apod/image/9706/fbgalax_hst_big.jpg,image,v1,Distant Galaxies,https://apod.nasa.gov/apod/image/9706/fbgalax_hst.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2024-02-02,"This cosmic view shows off an otherwise faint emission nebula IC 410, captured under clear Netherlands skies with telescope and narrowband filters. Above and right of center you can spot two remarkable inhabitants of the interstellar pond of gas and dust, known as the tadpoles of IC 410. Partly obscured by foreground dust, the nebula itself surrounds NGC 1893, a young galactic cluster of stars. Formed in the interstellar cloud a mere 4 million years ago, the intensely hot, bright cluster stars energize the glowing gas. Globules composed of denser cooler gas and dust, the tadpoles are around 10 light-years long and are likely sites of ongoing star formation. Sculpted by stellar winds and radiation their heads are outlined by bright ridges of ionized gas while their tails trail away from the cluster's central young stars. IC 410 and embedded NGC 1893 lie some 10,000 light-years away, toward the nebula-rich constellation Auriga.",https://apod.nasa.gov/apod/image/2402/Tadpoles2048original.png,image,v1,NGC 1893 and the Tadpoles of IC 410,https://apod.nasa.gov/apod/image/2402/Tadpoles1024original.png,Sander de Jong,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2004-12-19,"Where did all the stars go? What used to be considered a hole in the sky is now known to astronomers as a dark molecular cloud. Here, a high concentration of dust and molecular gas absorb practically all the visible light emitted from background stars. The eerily dark surroundings help make the interiors of molecular clouds some of the coldest and most isolated places in the universe. One of the most notable of these dark absorption nebulae is a cloud toward the constellation Ophiuchus known as Barnard 68, pictured above. That no stars are visible in the center indicates that Barnard 68 is relatively nearby, with measurements placing it about 500 light-years away and half a light-year across. It is not known exactly how molecular clouds like Barnard 68 form, but it is known that these clouds are themselves likely places for new stars to form. It is possible to look right through the cloud in infrared light.",https://apod.nasa.gov/apod/image/0109/barnard68_vlt_big.jpg,image,v1,Molecular Cloud Barnard 68,https://apod.nasa.gov/apod/image/0109/barnard68_vlt.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2009-03-24,"Human made robots continue to roll across the surface of Mars. Both Opportunity and its sister rover Spirit are in their sixth year on Mars, exploring the red planet for years longer than original expectations. Pictured above is a composite of recent images taken by the navigation camera on top of the Opportunity rover in Meridiani Planum. Visible are parallel rover tracks, rippling sand dunes, light-colored bedrock protrusions, metallic rover parts, and the dark shadow of the sometimes-artistic robotic photographer. Currently, Opportunity is on its way toward huge Endeavor crater, while Spirit is trying to climb an unusual rock structure known as Home Plate. If it can survive the harsh martian environment, Opportunity should arrive at Endeavor crater in about two years, at which time it may revolutionize human knowledge of this ancient martian landform.",https://apod.nasa.gov/apod/image/0903/windmars_opportunity_big.jpg,image,v1,Martian Dunes and the Shadow of Opportunity,https://apod.nasa.gov/apod/image/0903/windmars_opportunity.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2023-05-15,"From afar, the whole thing looks like an eagle. A closer look at the Eagle Nebula, however, shows the bright region is actually a window into the center of a larger dark shell of dust. Through this window, a brightly-lit workshop appears where a whole open cluster of stars is being formed. In this cavity, tall pillars and round globules of dark dust and cold molecular gas remain where stars are still forming. Already visible are several young bright blue stars whose light and winds are burning away and pushing back the remaining filaments and walls of gas and dust. The Eagle emission nebula, tagged M16, lies about 6500 light years away, spans about 20 light-years, and is visible with binoculars toward the constellation of the Serpent (Serpens). This picture involved long and deep exposures and combined three specific emitted colors emitted by sulfur (colored as yellow), hydrogen (red), and oxygen (blue).",https://apod.nasa.gov/apod/image/2305/EagleDeep_Lacroce_2047.jpg,image,v1,M16: Eagle Nebula Deep Field,https://apod.nasa.gov/apod/image/2305/EagleDeep_Lacroce_1080.jpg," -Gianni Lacroce -",exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2003-10-30,"Vivid auroral displays were triggered by a cloud of high energy particles and magnetic fields from the Sun that collided with planet Earth's magnetosphere yesterday, October 29, at about 06:30 Universal Time. The collision was anticipated, following an intense solar flare and coronal mass ejection detected on October 28, and many anxious skywatchers were rewarded with an enjoyable light show. While aurorae don't normally haunt skies in the southern United States, they were reported from locations in Missouri, Texas, New Mexico, and California in the early morning hours. Near Yampa, Colorado astronomer Jimmy Westlake also spent early yesterday morning enjoying the stormy space weather. He was impressed by this colorful apparition of the northern lights -- produced by oxygen and nitrogen atoms excited by collisions with energetic particles from the magnetosphere and returning to lower energy states, at altitudes of 100 kilometers or more. Brighter stars shine through the extreme high-altitude glow which shows much lower clouds and the distant horizon in silhouette.",https://apod.nasa.gov/apod/image/0310/aurora031029b_westlake_full.jpg,image,v1,Aurora in Colorado Skies,https://apod.nasa.gov/apod/image/0310/aurora031029b_westlake_c1.jpg," -Jimmy Westlake -(Colorado -Mountain College) +Jim and Janet Castano, +Adam Block, +NOAO, +AURA, +NSF +",exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +2015-01-27,"What does the magnetic field of our Galaxy look like? It has long been known that a modest magnetic field pervades our Milky Way Galaxy because it is seen to align small dust grains that scatter background light. Only recently, however, has the Sun-orbiting Planck satellite made a high-resolution map of this field. Color coded, the 30-degree wide map confirms, among other things, that the Galaxy's interstellar magnetism is strongest in the central disk. The revolution of charged gas around the Galactic center creates this magnetism, and it is hypothesized that viewed from the top, the Milky Way's magnetic field would appear as a spiral swirling out from the center. What caused many of the details in this and similar Planck maps -- and how magnetism in general affected our Galaxy's evolution -- will likely remain topics of research for years to come.",https://apod.nasa.gov/apod/image/1501/GalacticMagneticField_planck_3197.jpg,image,v1,Our Galaxy's Magnetic Field from Planck,https://apod.nasa.gov/apod/image/1501/GalacticMagneticField_planck_960.jpg," +ESA/Planck; + Acknowledgement: +M.-A. Miville-Desch�nes, CNRS � +IAS, +U. Paris-XI +",exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +2005-02-21,"Was the brightest Galactic blast yet recorded a key to connecting two types of celestial explosions? Last December, a dense sheet of gamma rays only a few times wider than the Earth plowed through our Solar System, saturating satellites and noticeably reflecting off the Moon. A magnetar near our Galactic Center, the source of Soft Gamma Repeater (SGR) 1806-20, had unleashed its largest flare on record. The brightness and briefness of the tremendous explosion's initial peak made it look quite similar to another type of tremendous explosion if viewed from further away -- a short duration gamma-ray burst (GRB). Short duration GRBs are thought by many to be fundamentally different than their long duration GRB cousins that are likely related to distant supernovas. Illustrated above is a series of drawings depicting an outgoing explosion during the initial SGR spike. A fast moving wave of radiation is pictured shooting away from a central magnetar. The possible link between SGRs and GRBs should become better understood as more and similar events are detected by the Earth-orbiting Swift satellite.",https://apod.nasa.gov/apod/image/0502/magnetarburst_mallozzi_big.jpg,image,v1,Galactic Magnetar Throws Giant Flare,https://apod.nasa.gov/apod/image/0502/magnetarburst_mallozzi.jpg," +Robert Mallozzi +(UAH, +MSFC) +",exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +2000-06-15,"The Perseus Cluster of thousands of galaxies, 320 million light-years distant, is one of the most massive objects in the Universe. At its core lies the giant cannibal galaxy Perseus A (NGC 1275), accreting matter as gas and galaxies fall into it. Representing low, medium, and high energy x-rays as red, green, and blue colours respectively, this Chandra X-ray Observatory image shows remarkable details of x-ray emission from this monster galaxy and surrounding hot (30-70 million degrees C) cluster gas. The bright central source is the supermassive black hole at the core of Perseus A itself. Dark circular voids just above and below the galaxy center, each about half the size of our own Milky Way Galaxy, are believed to be magnetic bubbles of energetic particles blown by the accreting black hole. Settling toward Perseus A, the cluster's x-ray hot gas piles up forming bright regions around the bubble rims. Dramatically, the long greenish wisp just above the galaxy's centre is likely the x-ray shadow produced by a small galaxy falling into the burgeoning Perseus A.",https://apod.nasa.gov/apod/image/0006/perseus_fabian_orig.jpg,image,v1,X-rays From The Perseus Cluster Core,https://apod.nasa.gov/apod/image/0006/perseus_fabiancxo.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +1995-10-26,,https://apod.nasa.gov/apod/image/aurora_shuttletail.gif,image,v1,Aurora Astern,https://apod.nasa.gov/apod/image/aurora_shuttletail.gif,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +2021-12-19,"It is not a coincidence that planets line up. That's because all of the planets orbit the Sun in (nearly) a single sheet called the plane of the ecliptic. When viewed from inside that plane -- as Earth dwellers are likely to do -- the planets all appear confined to a single band. It is a coincidence, though, when three of the brightest planets all appear in nearly the same direction. Such a coincidence was captured earlier this month. Featured above (right to left), Venus, Saturn, and Jupiter were all imaged together in a line just after sunset, from the San Fermo Hills, Bergamo, Italy. Joining the alignment are Earth's Moon, and the position of the more distant Uranus. Bands of clouds streak across the sky toward the setting Sun. As Comet Leonard fades, this planetary alignment -- absent the Moon -- should persist for the rest of the month. Discovery + Outreach: Graduate student research position open for APOD",https://apod.nasa.gov/apod/image/2112/PlanetsAligned_Finazzi_3757.jpg,image,v1,Planetary Alignment over Italy,https://apod.nasa.gov/apod/image/2112/PlanetsAligned_Finazzi_1080.jpg," +Antonio Finazzi +",exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +2022-12-17,"Get out your red/blue glasses and check out this stereo scene from Taurus-Littrow valley on the Moon! The color anaglyph features a detailed 3D view of Apollo 17's Lunar Rover in the foreground -- behind it lies the Lunar Module and distant lunar hills. Because the world was going to be able to watch the Lunar Module's ascent stage liftoff via the rover's TV camera, this parking place was also known as the VIP Site. Fifty years ago, in December of 1972, Apollo 17 astronauts Eugene Cernan and Harrison Schmitt spent about 75 hours on the Moon, while colleague Ronald Evans orbited overhead. The crew returned with 110 kilograms of rock and soil samples, more than from any of the other lunar landing sites. Cernan and Schmitt are still the last to walk (or drive) on the Moon.",https://apod.nasa.gov/apod/image/2212/a17anaglyph_vanMeijgaarden_f.jpg,image,v1,Apollo 17 VIP Site Anaglyph,https://apod.nasa.gov/apod/image/2212/a17anaglyph_vanMeijgaarden_1024v.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +2009-10-25,"This is the mess that is left when a star explodes. The Crab Nebula, the result of a supernova seen in 1054 AD, is filled with mysterious filaments. The filaments are not only tremendously complex, but appear to have less mass than expelled in the original supernova and a higher speed than expected from a free explosion. The above image, taken by the Hubble Space Telescope, is presented in three colors chosen for scientific interest. The Crab Nebula spans about 10 light-years. In the nebula's very center lies a pulsar: a neutron star as massive as the Sun but with only the size of a small town. The Crab Pulsar rotates about 30 times each second.",https://apod.nasa.gov/apod/image/0910/crabmosaic_hst_big.jpg,image,v1,M1: The Crab Nebula from Hubble,https://apod.nasa.gov/apod/image/0910/crabmosaic_hst.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +2018-05-04,"Big, beautiful spiral galaxy M101 is one of the last entries in Charles Messier's famous catalog, but definitely not one of the least. About 170,000 light-years across, this galaxy is enormous, almost twice the size of our own Milky Way galaxy. M101 was also one of the original spiral nebulae observed by Lord Rosse's large 19th century telescope, the Leviathan of Parsontown. M101 shares this modern telescopic field of view with spiky foreground stars within the Milky Way and a companion dwarf galaxy NGC 5474 (lower right). The colors of the Milky Way stars can also be found in the starlight from the large island universe. Its core is dominated by light from cool yellowish stars. Along its grand design spiral arms are the blue colors of hotter, young stars mixed with obscuring dust lanes and pinkish star forming regions. Also known as the Pinwheel Galaxy, M101 lies within the boundaries of the northern constellation Ursa Major, about 23 million light-years away. NGC 5474 has likely been distorted by its past gravitational interactions with the dominant M101.",https://apod.nasa.gov/apod/image/1805/M101_3Days_New_APOD.jpg,image,v1,The View Toward M101,https://apod.nasa.gov/apod/image/1805/M101_3Days_New_APOD1024.jpg,Joonhwa Lee,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +2004-07-23,"What colors are Saturn's rings? Recent images from the Cassini spacecraft now orbiting Saturn confirm that different rings have slightly different colors. The above image shows their sometimes-subtle differences in brightness and color. The rings reflect sunlight and so, even if they were perfectly reflecting, would appear the color of the Sun. The ring particles are mostly light water-ice, although these particles can be shaded by an unknown type of darker dirt. Thinner and more isolated rings also naturally appear darker. The brightest section pictured above is Saturn's B ring.",https://apod.nasa.gov/apod/image/0407/colorrings_cassini_big.jpg,image,v1,Saturn's Rings in Natural Color,https://apod.nasa.gov/apod/image/0407/colorrings_cassini.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +2022-02-01,"What will the Moon phase be on your birthday this year? It is hard to predict because the Moon's appearance changes nightly. As the Moon orbits the Earth, the half illuminated by the Sun first becomes increasingly visible, then decreasingly visible. The featured video animates images and altitude data taken by NASA's Moon-orbiting Lunar Reconnaissance Orbiter to show all 12 lunations that appear this year, 2022 -- as seen from Earth's northern (southern) hemisphere. A single lunation describes one full cycle of our Moon, including all of its phases. A full lunation takes about 29.5 days, just under a month (moon-th). As each lunation progresses, sunlight reflects from the Moon at different angles, and so illuminates different features differently. During all of this, of course, the Moon always keeps the same face toward the Earth. What is less apparent night-to-night is that the Moon's apparent size changes slightly, and that a slight wobble called a libration occurs as the Moon progresses along its elliptical orbit.",,video,v1,Moon Phases 2022,https://www.youtube.com/embed/c4Xky6tlFyY?rel=0&VQ=HD720,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +2014-12-28,"What's happening over that town? Close inspection shows these strange columns of light occur over bright lights, and so likely are light pillars that involve falling ice crystals reflecting back these lights. The above image and several similar images were taken with a standard digital camera in Sigulda, Latvia in late 2009. The reason why these pillars fan out at the top, however, remains a topic for speculation. The air was noted to be quite cold and indeed filled with small ice crystals, just the type known to create several awe-inspiring but well known sky phenomena such as light pillars, sun pillars, sun dogs, and moon halos. The cold and snowy winter occurring this year in parts of Earth's northern hemisphere is giving sky enthusiasts new and typically unexpected opportunities to see several of these unusual optical atmospheric phenomena for themselves.",https://apod.nasa.gov/apod/image/1412/icepillar_truhin_1715.jpg,image,v1,Unusual Light Pillars over Latvia,https://apod.nasa.gov/apod/image/1412/icepillar_truhin_960.jpg,Aigar Truhin,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +1995-07-12,"July 12, 1995 Eta Carinae Before Explosion Picture Credit: NASA, HST, WFPC2, J. Hester (ASU) Explanation: The star Eta Carinae, at the center of the photo, will likely destroy itself in a spectacular explosion in a few million years - or sooner! Currently it is one of the brightest, most massive, and least stable stars known. Much of the gas in this Hubble Space Telescope photograph was blown off the star itself. Some of these gas clouds are similar in size to our solar system. Astronomers cannot yet fully explain the motions of the surrounding nebula, and continue to study this system. Reference: the Space Telescope Scientific Institute's press release. We keep an archive of Astronomy Pictures of the Day. Astronomy Picture of the Day is brought to you by Robert Nemiroff and Jerry Bonnell . Original material on this page is copyrighted to Robert J. Nemiroff and Jerry T. Bonnell.",https://apod.nasa.gov/apod/image/etacarinae_hst.gif,image,v1,Eta Carinae Before Explosion,https://apod.nasa.gov/apod/image/etacarinae_hst.gif,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +2005-05-21,"Dark nebulae snake across a gorgeous expanse of stars in this wide-field view toward the pronounceable constellation Ophiuchus and the center of our Milky Way Galaxy. In fact, the central S-shape seen here is well known as the Snake Nebula. It is also listed as Barnard 72 (B72), one of 182 dark markings of the sky cataloged in the early 20th century by astronomer E. E. Barnard. Unlike bright emission nebulae and star clusters, Barnard's nebulae are interstellar dark clouds of obscuring gas and dust. Their shapes are visible in cosmic silhouette only because they lie in the foreground along the line of sight to rich star fields and glowing stellar nurseries near the plane of our Galaxy. Many of Barnard's dark nebulae are themselves likely sites of future star formation. Barnard 72 is a few light years across and about 650 light years away.",https://apod.nasa.gov/apod/image/0505/b72neb_stevens_full.jpg,image,v1,Snake in the Dark,https://apod.nasa.gov/apod/image/0505/b72neb_stevens_c1.jpg," +Gary Stevens +",exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +2015-07-24,"A mere 2.5 million light-years away the Andromeda Galaxy, also known as M31, really is just next door as large galaxies go. So close and spanning some 260,000 light-years, it took 11 different image fields from the Galaxy Evolution Explorer (GALEX) satellite's telescope to produce this gorgeous portrait of the spiral galaxy in ultraviolet light. While its spiral arms stand out in visible light images of Andromeda, the arms look more like rings in the GALEX ultraviolet view, a view dominated by the energetic light from hot, young, massive stars. As sites of intense star formation, the rings have been interpreted as evidence Andromeda collided with its smaller neighboring elliptical galaxy M32 more than 200 million years ago. The large Andromeda galaxy and our own Milky Way are the most massive members of the local galaxy group.",https://apod.nasa.gov/apod/image/1507/AndromedaGalex_2048.jpg,image,v1,Ultraviolet Rings of M31,https://apod.nasa.gov/apod/image/1507/AndromedaGalex_900.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +2001-10-28,"It may look like a butterfly, but it's bigger than our Solar System. NGC 2346 is a planetary nebula made of gas and dust that has evolved into a familiar shape. At the heart of the bipolar planetary nebula is a pair of close stars orbiting each other once every sixteen days. The tale of how the butterfly blossomed probably began millions of years ago, when the stars were farther apart. The more massive star expanded to encompass its binary companion, causing the two to spiral closer and expel rings of gas. Later, bubbles of hot gas emerged as the core of the massive red giant star became uncovered. In billions of years, our Sun will become a red giant and emit a planetary nebula - but probably not in the shape of a butterfly, because the Sun has no binary star companion.",https://apod.nasa.gov/apod/image/0110/ngc2346_heritage_big.jpg,image,v1,NGC 2346: A Butterfly-Shaped Planetary Nebula,https://apod.nasa.gov/apod/image/0110/ngc2346_heritage.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +2001-10-05,"Only a few stars can be found within ten light-years of our lonely Sun, situated near an outer spiral arm of the Milky Way galaxy. But if the Sun were found within one of our galaxy's star clusters, thousands of stars might occupy a similar space. What would the night sky look like in such a densely packed stellar neighborhood? When Roger Hopkins took this picture at the Montezuma National Wildlife Refuge in the Finger Lakes region of western New York, USA, he was struck by this same notion. Appropriately, he had photographed a flock of starlings against the backdrop of a serene sunset. He then manipulated the image so that the black bird silhouettes were changed to white. The final picture dramatically suggests the tantalizing spectacle of approaching night in crowded skies above a cluster star world.",https://apod.nasa.gov/apod/image/0110/whitebirds640_rhopkins.jpg,image,v1,A Flock of Stars,https://apod.nasa.gov/apod/image/0110/whitebirds640_rhopkins.jpg," +Roger A. Hopkins +",exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +2010-01-30,"Charles Messier described the 88th entry in his 18th century catalog of Nebulae and Star Clusters as a spiral nebula without stars. Of course the gorgeous M88 is now understood to be a galaxy full of stars, gas, and dust, not unlike our own Milky Way. In fact, M88 is one of the brightest galaxies in the Virgo Galaxy Cluster some 50 million light-years away. M88's beautiful spiral arms are easy to trace in this colorful cosmic portait. The arms are lined with young blue star clusters, pink star-forming regions, and obscuring dust lanes extending from a yellowish core dominated by an older population of stars. Spiral galaxy M88 spans over 100,000 light-years.",https://apod.nasa.gov/apod/image/1001/m88ms_block_crop.jpg,image,v1,Messier 88,https://apod.nasa.gov/apod/image/1001/m88ms_block_c900.jpg,Adam Block,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +2013-04-04,"This beautiful, bright, spiral galaxy is Messier 64, often called the Black Eye Galaxy or the Sleeping Beauty Galaxy for its heavy-lidded appearance in telescopic views. M64 is about 17 million light-years distant in the otherwise well-groomed northern constellation Coma Berenices. In fact, the Red Eye Galaxy might also be an appropriate moniker in this colorful composition of narrow and wideband images. The enormous dust clouds obscuring the near-side of M64's central region are laced with the telltale reddish glow of hydrogen associated with star forming regions. But they are not this galaxy's only peculiar feature. Observations show that M64 is actually composed of two concentric, counter-rotating systems. While all the stars in M64 rotate in the same direction as the interstellar gas in the galaxy's central region, gas in the outer regions, extending to about 40,000 light-years, rotates in the opposite direction. The dusty eye and bizarre rotation is likely the result of a billion year old merger of two different galaxies.",https://apod.nasa.gov/apod/image/1304/M64HaLRGB_Pugh.jpg,image,v1,M64: The Black Eye Galaxy,https://apod.nasa.gov/apod/image/1304/M64HaLRGB_Pugh920.jpg,Martin Pugh,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +2005-02-16,"Sunspots -- magnets the size of the Earth -- are normally seen flat on the Sun. The above digital metamorphosis, however, shows a sunspot as it appears at increasing heights, effectively in three dimensions. The above false-colored image sequence of solar active region AR 10675 was taken in three very specific colors that effectively isolate different layers above the solar surface. The first images show the Sun's photospheric surface as it normally appears, covered with granules. The large dark sunspot sports a clear dark umbra in the center surrounded by a lighter penumbra. Images appearing toward the middle of the sequence show the Sun as in light predominantly emitted a few hundred kilometers above the photosphere. At this height, the continent sized bubbling granules appear reversed, and long lines of constant magnetic force begin to appear. The last images show the Sun at a few thousand kilometers into the chromosphere. Here magnetic field lines can be clearly followed outward from the sunspot to distant regions.",https://apod.nasa.gov/apod/image/0502/spotmorph_dot_big.gif,image,v1,Sunspot Metamorphosis: From Bottom to Top,https://apod.nasa.gov/apod/image/0502/spotmorph_dot.gif,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +2021-09-28,"Have you ever experienced a meteor shower? To help capture the wonder, a video was taken during the peak of the recent Perseid meteor shower above the Indian Astronomical Observatory in Hanle, India, high up in the Himalayan mountains. Night descends as the video begins, with the central plane of our Milky Way Galaxy approaching from the left and Earth-orbiting satellites zipping by overhead. During the night, the flash of meteors that usually takes less than a second is artificially extended. The green glow of most meteors is typically caused by vaporizing nickel. As the video continues, Orion rises and meteors flare above the 2-meter Himalayan Chandra Telescope and the seven barrels of the High Energy Gamma Ray Telescope (Hagar). The 2 minute 30 second movie ends with the Sun rising, preceded by a false dawn of zodiacal light.",,video,v1,Night of the Perseids,https://www.youtube.com/embed/tLC6Sy8f06s?rel=0," +Vikas Chander & Dorje Angchuk; + Music: Tea Time via PremiumBeat +",exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +2014-06-06,"Sweeping slowly through northern skies, the comet PanSTARRS C/2012 K1 posed for this telescopic portrait on June 2nd in the constellation Ursa Major. Now within the inner solar system, the icy body from the Oort cloud sports two tails, a lighter broad dust tail and crooked ion tail extending below and right. The comet's condensed greenish coma makes a nice contrast with the spiky yellowish background star above. NGC 3319 appears at the upper left of the frame that spans almost twice the apparent diameter of the full Moon. The spiral galaxy is about 47 million light-years away, far beyond the stars in our own Milky Way. In comparison, the comet was a mere 14 light-minutes from our fair planet. This comet PanSTARRS will slowly grow brighter in the coming months remaining a good target for telescopic comet watchers and reaching perihelion, its closest approach to the Sun, while just beyond Earth's orbit in late August.",https://apod.nasa.gov/apod/image/1406/PanstarssN3319Falesiedi.jpg,image,v1,Comet PanSTARRS with Galaxy,https://apod.nasa.gov/apod/image/1406/PanstarssN3319Falesiedi950.jpg,Alessandro Falesiedi,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +2009-04-17,"Discovered by accident, this manuscript page provides graphical insight to astronomy in medieval times, before the Renaissance and the influence of Nicolaus Copernicus, Tycho de Brahe, Johannes Kepler, and Galileo. The intriguing page is from lecture notes on astronomy compiled by the monk Magister Wolfgang de Styria before the year 1490 at Melk Abbey in Austria. The top panels clearly illustrate the necessary geometry for a lunar (left) and solar eclipse in the Earth-centered Ptolemaic system. At lower left is a diagram of the Ptolemaic view of the solar system and at the lower right is a chart to calculate the date of Easter Sunday in the Julian calendar. Text at the upper right explains the movement of the planets according to the Ptolemaic system. The actual manuscript page is on view at historic Melk Abbey as part of a special exhibition during the International Year of Astronomy.",https://apod.nasa.gov/apod/image/0904/medieval_fragment50p.jpg,image,v1,Medieval Astronomy from Melk Abbey,https://apod.nasa.gov/apod/image/0904/medieval_fragmentW600.jpg,"Library of Melk Abbey, Frag. 229 -",exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2002-07-11,"Fresh from yesterday's episode, a popular pair of interacting galaxies known as the Whirlpool debut here beyond the realm of visible light -- imaged at high energies by the orbiting Chandra X-ray Observatory. Still turning in a remarkable performance, over 80 glittering x-ray stars are present in the Chandra image data from the region. The number of luminous x-ray sources, likely neutron star and black hole binary systems within the confines of M51, is unusually high for normal spiral or elliptical galaxies and suggests this cosmic whirlpool has experienced intense bursts of massive star formation. The bright cores of both galaxies, NGC 5194 and NGC 5195 (right and left respectively), also exhibit high-energy activity in this false-color x-ray picture showing a diffuse glow from multi-million degree gas. An expanded view of the region near the core of NGC 5194 reveals x-rays from a supernova remnant, the debris from a spectacular stellar explosion, first detected by earthbound astronomers in 1994.",https://apod.nasa.gov/apod/image/0207/m51_cxc_big.jpg,image,v1,M51: X-Rays from the Whirlpool,https://apod.nasa.gov/apod/image/0207/m51_cxc.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2005-06-09,"This serene image of boats moored in the harbor of l'�le-Tudy, Bretagne, France was taken on June 1st, about an hour after sunset. It also features Venus, third brightest celestial object after the Sun and Moon. For casual skygazers, this month marks Venus' return to the evening sky as the brilliant 'star', shining low in the west-northwest shortly after sunset. In the picture, astrophotographer and APOD translator Laurent Laveder notes that Venus is easily mistaken for a light atop a sailboat's tall mast, giving the otherwise stunning celestial beacon an unremarkable appearance. Of course, a year ago Venus' appearance was quite remarkable. On June 8, 2004, Venus crossed the Sun's disk, the first transit of Venus since 1882. Late this week Venus shares the evening sky with the young crescent Moon, and will next transit the Sun on June 6, 2012.",https://apod.nasa.gov/apod/image/0506/venusret_laveder_full.jpg,image,v1,Venus Returns to the Evening Sky,https://apod.nasa.gov/apod/image/0506/venusret_laveder_c65.jpg," -Laurent Laveder -(Version -fran�aise officielle de l'APOD) +",exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +2004-05-06,"From start to finish, this impressive digital mosaic covers May 4th's total eclipse of the Moon. Astronomer Anthony Ayiomamitis reports that the eclipse viewing was wonderful from Greece, where skies cleared shortly before the celestial show began. His mosaic includes images, recorded at five minute intervals and arranged sequentially in an arc, that trace the progress of the inner portion of the Earth's shadow or umbra across the lunar disk. A series depicting a surprisingly dark, totally eclipsed Moon is featured in the center. While May 4th's total lunar eclipse favored observers in Europe, Africa, and Asia, the Moon's next trip through Earth's shadow, scheduled for October 28, will give skygazers in the Americas a turn.",https://apod.nasa.gov/apod/image/0405/tle_may2004_ayiomamitis.jpg,image,v1,A Lunar Eclipse Mosaic,https://apod.nasa.gov/apod/image/0405/tle_may2004_ayiomamitis.jpg," +Anthony Ayiomamitis +",exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +1998-09-15,"What happens if you point a large telescope at nothing? The above New Technology Telescope SUSI Deep Field photograph isolated a small patch of sky picked to contain no bright objects at all. A very long exposure was then taken, similar to the Hubble Deep Field, in order to see the many faint objects that are usually washed out by the light of bright foreground objects. What remains is a cosmic wallpaper rich in distant galaxies. Galaxies as faint as magnitude 26 were found to be irregularly distributed, with several unusual pairings of different colored objects. This and other deep field images are being released for detailed inspection by anyone interested. New deep field images are being planned.",https://apod.nasa.gov/apod/image/9809/deepfield_ntt_big.jpg,image,v1,The NTT SUSI Deep Field,https://apod.nasa.gov/apod/image/9809/deepfield_ntt.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +2019-12-11,"What has this supernova left behind? As little as 2,000 years ago, light from a massive stellar explosion in the Large Magellanic Cloud (LMC) first reached planet Earth. The LMC is a close galactic neighbor of our Milky Way Galaxy and the rampaging explosion front is now seen moving out - destroying or displacing ambient gas clouds while leaving behind relatively dense knots of gas and dust. What remains is one of the largest supernova remnants in the LMC: N63A. Many of the surviving dense knots have been themselves compressed and may further contract to form new stars. Some of the resulting stars may then explode in a supernova, continuing the cycle. Featured here is a combined image of N63A in the X-ray from the Chandra Space Telescope and in visible light by Hubble. The prominent knot of gas and dust on the upper right -- informally dubbed the Firefox -- is very bright in visible light, while the larger supernova remnant shines most brightly in X-rays. N63A spans over 25 light years and lies about 150,000 light years away toward the southern constellation of Dorado.",https://apod.nasa.gov/apod/image/1912/N63A_HubbleChandraSchmidt_1019.jpg,image,v1,N63A: Supernova Remnant in Visible and X-ray,https://apod.nasa.gov/apod/image/1912/N63A_HubbleChandraSchmidt_960.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +1996-08-15,"Io's surface is active. Geyser-like eruptions from volcanoes on this Jovian moon were seen by both Voyager spacecraft in 1979 and were also spotted this year in late June by Galileo's camera from a distance of about 600,000 miles. The blue plume seen at the moon's edge (magnified in the inset) arises from Ra Patera, a large shield volcano, and extends about 60 miles above the surface. The blue color is attributed to condensing and freezing sulfur dioxide gas. Galileo images have also revealed that the plume glows in the dark - perhaps due to fluorescence of excited sulfur and oxygen ions. Io's surface is cold, its temperature averages about -230 degrees Fahrenheit, so why is it so active? The most likely cause is the gravitational tug of war over Io between Jupiter and the other Galilean moons which perturbs Io's orbit. The orbital changes would result in tidal force variations heating Io's interior and and generating the sulfurous volcanic activity.",https://apod.nasa.gov/apod/image/iovol2_gal_big.jpg,image,v1,Galileo Views Io Eruption,https://apod.nasa.gov/apod/image/iovol2_gal.gif,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +2007-08-12,"Tonight is a good night to see meteors. Comet dust will rain down on planet Earth, streaking through dark skies in the annual Perseid meteor shower. While enjoying the anticipated space weather, astronomer Fred Bruenjes recorded a series of many 30 second long exposures spanning about six hours on the night of 2004 August 11/12 using a wide angle lens. Combining those frames which captured meteor flashes, he produced this dramatic view of the Perseids of summer. Although the comet dust particles are traveling parallel to each other, the resulting shower meteors clearly seem to radiate from a single point on the sky in the eponymous constellation Perseus. The radiant effect is due to perspective, as the parallel tracks appear to converge at a distance. Bruenjes notes that there are 51 Perseid meteors in the composite image, including one seen nearly head-on. This year, the Perseids Meteor Shower is expected to peak after midnight tonight, in the moonless early morning hours of August 12.",https://apod.nasa.gov/apod/image/0708/perseids_bruenjes_big.jpg,image,v1,Raining Perseids,https://apod.nasa.gov/apod/image/0708/perseids_bruenjes.jpg," +Fred Bruenjes +",exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +1998-12-31,"Distant supernovae were among topics at the forefront of astronomy during 1998. Two independent groups raced to deploy large telescopes to scan the sky, discovering and analyzing far-off supernovae with the promise of calibrating the geometry of our universe. The results were surprising -- implying an unexpected universe rich in not only dark matter (Omega in matter ~ 0.3) but also in dark energy (Lambda ~ 0.7). Skeptics remain cautious, however, some waiting for more than a few high- redshift supernovae to light the way, while others waiting for verification methods not vulnerable to the same types of systematic errors. Pictured above are several of the distant supernovae that have ignited modern cosmology.",https://apod.nasa.gov/apod/image/9812/sne98_hiz_big.jpg,image,v1,The Year of Distant Supernovae,https://apod.nasa.gov/apod/image/9812/sne98_hiz.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +1997-03-23,"Comet Shoemaker-Levy 9, named after its co-discoverers, was often referred to as the ""string of pearls"" comet. It is famous for its unusual appearance as well as its collision with the planet Jupiter! The comet's original single nucleus was torn to pieces by Jupiter's strong gravity during a close encounter with the solar system's largest planet in 1992. The pieces are seen in this composite of Hubble Space Telescope images to be ""pearls"" strung out along the comet's orbital path. In July of 1994 these pieces collided with Jupiter in a rare and spectacular series of events.",https://apod.nasa.gov/apod/image/9703/sl9_hst_big.jpg,image,v1,"A String Of Pearls +Credit:",https://apod.nasa.gov/apod/image/9703/sl9_hst.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +2007-04-21,"Get out your red/blue glasses and gaze down on this weathered mesa on Mars. Of course, described as a rock formation that resembles a human head in a 1976 NASA press release, this mesa is also famous as the Face on Mars. The sharp stereo image was created by combining high resolution pictures from cameras on two different spacecraft in Mars orbit - Mars Reconnaissance Orbiter and Mars Global surveyor. It shows rugged details of the approximately 2 kilometer wide, isolated hill - similar to mesa landforms on planet Earth - rising some 240 meters above the plains of the martian Cydonia region. This remarkable 3D view exaggerates the hill's vertical dimensions.",https://apod.nasa.gov/apod/image/0704/MRO-GS-vantuyne.jpg,image,v1,3D Face on Mars,https://apod.nasa.gov/apod/image/0704/MRO-GS-vantuyne720.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +1997-05-08,"This enhanced composite image detailing structure in the coma and dust tail of Hale-Bopp was recorded May 5 - one day before the comet's passage from north to south across the plane of Earth's orbit. As the comet descends into murky twilight for northern hemisphere observers it will become increasingly easy to view from the south. Along with Southern Hemisphere observers, astronomers and a fleet of spacecraft of the International Solar-Terrestrial Physics program have been anxiously awaiting this north/south crossing. The comet's interaction with the changing equatorial solar wind and magnetic field during this crossing is expected to produce distortions and disconnections of Hale-Bopp's ion tail. Whisker-like structures, probably part of the ion tail, are visible above extending from the lower left of the bright coma.",https://apod.nasa.gov/apod/image/9705/hb_puckett5_big.jpg,image,v1,"Detailing Hale-Bopp +Credit and Copyright:",https://apod.nasa.gov/apod/image/9705/hb_puckett5.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +1999-08-02,Tomorrow's picture: Vela Expands < Archive | Index | Search | Calendar | Glossary | Education | About APOD > Authors & editors: Robert Nemiroff (MTU) & Jerry Bonnell (USRA) NASA Technical Rep.: Jay Norris. Specific rights apply. A service of: LHEA at NASA/ GSFC & Michigan Tech. U.,https://apod.nasa.gov/apod/image/9908/occult_orman_99.jpg,image,v1,Regulus Occulted,https://apod.nasa.gov/apod/image/9908/occult_orman_99.jpg," +Joe Orman +",exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +2023-12-16,"Peering from the shadows, the Saturn-facing hemisphere of tantalizing inner moon Enceladus poses in this Cassini spacecraft image. North is up in the dramatic scene captured during November 2016 as Cassini's camera was pointed in a nearly sunward direction about 130,000 kilometers from the moon's bright crescent. In fact, the distant world reflects over 90 percent of the sunlight it receives, giving its surface about the same reflectivity as fresh snow. A mere 500 kilometers in diameter, Enceladus is a surprisingly active moon. Data and images collected during Cassini's flybys have revealed water vapor and ice grains spewing from south polar geysers and evidence of an ocean of liquid water hidden beneath the moon's icy crust.",https://apod.nasa.gov/apod/image/2312/PIA20522enceladus.jpg,image,v1,Crescent Enceladus,https://apod.nasa.gov/apod/image/2312/PIA20522enceladusC.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +2004-10-24,"From afar, the whole thing looks like an Eagle. A closer look at the Eagle Nebula, however, shows the bright region is actually a window into the center of a larger dark shell of dust. Through this window, a brightly-lit workshop appears where a whole open cluster of stars is being formed. In this cavity tall pillars and round globules of dark dust and cold molecular gas remain where stars are still forming. Already visible are several young bright blue stars whose light and winds are burning away and pushing back the remaining filaments and walls of gas and dust. The Eagle emission nebula, tagged M16, lies about 6500 light years away, spans about 20 light-years, and is visible with binoculars toward the constellation of Serpens. The above picture combines three specific emitted colors and was taken with the 0.9-meter telescope on Kitt Peak, Arizona, USA.",https://apod.nasa.gov/apod/image/0206/eagle_kp09_big.jpg,image,v1,Inside the Eagle Nebula,https://apod.nasa.gov/apod/image/0206/eagle_kp09.jpg,T. A. Rector,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +2021-05-12,"Is the night sky darkest in the direction opposite the Sun? No. In fact, a rarely discernable faint glow known as the gegenschein (German for ""counter glow"") can be seen 180 degrees around from the Sun in an extremely dark sky. The gegenschein is sunlight back-scattered off small interplanetary dust particles. These dust particles are millimeter sized splinters from asteroids and orbit in the ecliptic plane of the planets. Pictured here from last March is one of the more spectacular pictures of the gegenschein yet taken. The deep exposure of an extremely dark sky over Teide Observatory in Spain's Canary Islands shows the gegenschein as part of extended zodiacal light. Notable background objects include a bright meteor (on the left), the Big Dipper (top right), and Polaris (far right). The meteor nearly points toward Mount Teide, Spain's highest mountain, while the Pyramid solar laboratory is visible on the right. During the day, a phenomenon like the gegenschein called the glory can be seen in reflecting air or clouds opposite the Sun from an airplane.",https://apod.nasa.gov/apod/image/2105/GegenscheinBolide_Casado_2500.jpg,image,v1,A Meteor and the Gegenschein,https://apod.nasa.gov/apod/image/2105/GegenscheinBolide_Casado_1080.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +2015-07-29,"Ridges of glowing interstellar gas and dark dust clouds inhabit the turbulent, cosmic depths of the Lagoon Nebula. Also known as M8, The bright star forming region is about 5,000 light-years distant. But it still makes for a popular stop on telescopic tours of the constellation Sagittarius, toward the center of our Milky Way Galaxy. Dominated by the telltale red emission of ionized hydrogen atoms recombining with stripped electrons, this stunning, deep view of the Lagoon's central reaches is about 40 light-years across. Near the center of the frame, the bright hourglass shape is gas ionized and sculpted by energetic radiation and extreme stellar winds from a massive young star.",https://apod.nasa.gov/apod/image/1507/block_m8_32ins.jpg,image,v1,The Deep Lagoon,https://apod.nasa.gov/apod/image/1507/block_m8_32ins1024.jpg,Adam Block,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +2012-08-14,"Where will the next Perseid meteor appear? Sky enthusiasts who trekked outside for the Perseid meteor shower that peaked over the past few days typically had this question on their mind. Six meteors from this past weekend are visible in the above stacked image composite, including one bright fireball streaking along the band of the background Milky Way Galaxy. All Perseid meteors appear to come from the shower radiant in the constellation of Perseus. Early reports about this year's Perseids indicate that as many as 100 meteors per hour were visible from some dark locations during the peak. The above digital mosaic was taken near Weikersheim, Germany. Growing Gallery: Perseid meteor shower images",https://apod.nasa.gov/apod/image/1208/perseids2012_hackmann_2000.jpg,image,v1,Perseid Meteors and the Milky Way,https://apod.nasa.gov/apod/image/1208/perseids2012_hackmann_960.jpg," +Jens Hackmann +",exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +2002-05-06,"These two galaxies are pulling each other apart. Known as ""The Mice"" because they have such long tails, each spiral galaxy has likely already passed through the other and will probably collide again and again until they coalesce. The long tails are created by the relative difference between gravitational pulls on the near and far parts of each galaxy. Scrolling right will show the very long tail of one of the galaxies. Because the distances are so large, the whole thing takes place in slow motion -- over hundreds of millions of years. NGC 4676 lies about 300 million light-years away toward the constellation of Coma Berenices and are likely members of the Coma Cluster of Galaxies. The above picture was taken with the Hubble Space Telescope's new Advanced Camera for Surveys which is more sensitive and images a larger field than previous Hubble cameras. The camera's increased sensitivity has imaged, serendipitously, galaxies far in the distance scattered about the frame.",https://apod.nasa.gov/apod/image/0205/ngc4676_hst_big.jpg,image,v1,NGC 4676: When Mice Collide,https://apod.nasa.gov/apod/image/0205/ngc4676_hst.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +2000-07-25,"This is what a star really looks like from the surface of the Earth. To the best the human eye can see, stars are so far away they appear the same as would infinitesimal points of light. The Earth's atmosphere, however, is clumpy, so that different air pockets produce different images of a single point-like star. Because the atmosphere is always windy and changing, the number and position of images is always changing, with the result that stars appear to twinkle. In reality, the above time-lapse sequence occurs ten times faster. Close inspection will reveal a single small image of the star that is repeated over and over. This image is called a speckle and its size is again not really infinitesimal, but determined by strange quantum effects that involve the finite size of the telescope. Recent work in adaptive optics (""rubber mirrors"") have made spectacular advances in reducing this atmospheric blurring. Betelgeuse is the star twinkling above, and in space, above the Earth's atmosphere, it really looks like this.",https://apod.nasa.gov/apod/image/0007/AlphaOri_cardiff.gif,image,v1,Why Stars Twinkle,https://apod.nasa.gov/apod/image/0007/AlphaOri_cardiff_big.gif,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +2011-04-19,"A symphony of planet-wide observations began abruptly on March 28 when the Earth-orbiting Swift satellite detected a burst of high-frequency gamma-rays from GRB 110328A. When the same source flared again after a 45 minute pause it was clear this event was not a typical gamma-ray burst. Twelve hours after the initial fanfare astronomers using the 2.5-meter Nordic Optical Telescope chimed in with a mid-range observation of the optical counterpart. Early the next day the explosion was picked up in baritone low-frequencies of radio waves by the EVLA radio dishes in the USA. Later many optical telescopes, including the 8-meter Gemini North telescope in Hawaii, began playing along by tracking the optical counterpart. The unusual source was spotted at a higher register in X-rays by the Chandra X-ray Observatory and was intermittently followed in the even more soprano-like gamma-ray range for a week. Joining the chorus, Hubble Space Telescope recorded this image in optical and infrared light, confirming that the flash was located along the path of a galaxy at redshift 0.351. If associated with the galaxy, this explosion occurred when the universe was about two thirds of its present age. There is much speculation that the unusual gamma-ray burst was a star being ripped apart by a supermassive black hole in the center of a galaxy and the puzzling features of the distant detonation are still being explored.",https://apod.nasa.gov/apod/image/1104/grb110328a_hst_3000.jpg,image,v1,The GRB 110328A Symphony,https://apod.nasa.gov/apod/image/1104/grb110328a_hst_900.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +1997-02-16,"Betelgeuse (sounds a lot like ""beetle juice""), a red supergiant star about 600 light years distant, is seen in this Hubble Space Telescope image -- the first direct picture of the surface of a star other than the Sun. A bright, as yet unexplained hotspot is revealed on its surface! While Betelgeuse is cooler than the Sun, it is more massive and over 1000 times larger. If placed at the center of our Solar System, it would extend past the orbit of Jupiter. Betelgeuse is also known as Alpha Orionis, one of the brightest stars in the familar constellation of Orion, the Hunter. Like many star names, Betelgeuse is Arabic in origin. It is derived from a phrase which refers to the hunter's shoulder or armpit, the general area occupied by this star in drawings of the figure in the constellation. As a massive red supergiant, it is nearing the end of its life and will soon become a supernova.",https://apod.nasa.gov/apod/image/9702/betelgeuse_hst_big.jpg,image,v1,"Betelgeuse, Betelgeuse, Betelgeuse -",exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2018-05-25,"This stunning group of galaxies is far, far away, about 450 million light-years from planet Earth and cataloged as galaxy cluster Abell S0740. Dominated by the cluster's large central elliptical galaxy (ESO 325-G004), this reprocessed Hubble Space Telescope view takes in a remarkable assortment of galaxy shapes and sizes with only a few spiky foreground stars scattered through the field. The giant elliptical galaxy (right of center) spans over 100,000 light years and contains about 100 billion stars, comparable in size to our own spiral Milky Way galaxy. The Hubble data can reveal a wealth of detail in even these distant galaxies, including arms and dust lanes, star clusters, ring structures, and gravitational lensing arcs.",https://apod.nasa.gov/apod/image/1805/ESO325-Pestana.jpg,image,v1,Galaxies Away,https://apod.nasa.gov/apod/image/1805/ESO325-Pestana1024.jpg,Hubble Legacy Archive,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2008-11-18,"Pictured above is the first image ever taken of the Earth from the Moon. The image was taken in 1966 by Lunar Orbiter 1 and heralded by then-journalists as the Image of the Century. It was taken about two years before the Apollo 8 crew snapped its more famous color cousin. Recently, modern technology has allowed the recovery of higher resolution images from old data sources such as Lunar Orbiter tapes than ever before. Specifically, recovery of the above image was initiated 20 years ago by Nancy Evans, and completed recently by Dennis Wingo and Keith Cowing who lead the Lunar Orbiter Image Recovery Project. Lunar Orbiter Image Recovery Project. Images like that above carry more than aesthetic value -- comparison to recent high definition images of the Moon enables investigations into how the Moon has been changing.",https://apod.nasa.gov/apod/image/0811/earthmoon_nasa_big.png,image,v1,Restored: First Image of the Earth from the Moon,https://apod.nasa.gov/apod/image/0811/earthmoon_nasa.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2011-03-14,"Have you ever seen a ""star"" drifting slowly overhead, but not known what it was? Sometimes even pointing it out to friends or family will only lead to a shrug. What you are seeing, most likely, is a spacecraft in low Earth orbit reflecting back sunlight as it circles the Earth once every 90 minutes or so. Two of the brighter spacecraft in the present day sky are the International Space Station (ISS), and, when it is up, a NASA space shuttle. As relative orientations change, the brightness of reflections may also change, sometimes suddenly. Another source of bright drifting objects, Iridium communication satellites, may even appear to flare up to become brighter than any other sky object for a few seconds. Pictured above, two bright points of light separated by only a few degrees drifted together across the sky above Lory State Park, Colorado, USA last week, just after sunset. These lights were were the ISS and the space shuttle Discovery, which had undocked from the ISS a few hours earlier. Given a digital fusion of many separate camera exposures and a wide angle perspective, the pair appears above as streaks in front of point-like stars. Web sites now exist that can help you identify unknown ""drifters"" and even predict the time of the next pass of the ISS visible from your location.",https://apod.nasa.gov/apod/image/1103/issshuttle_arn_2400.jpg,image,v1,Spacecrafts Streak Over Colorado,https://apod.nasa.gov/apod/image/1103/issshuttle_arn_900.jpg," -Robert Arn -",exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2009-09-26,"Our magnificent Milky Way Galaxy sprawls across this ambitious all-sky panorama. In fact, at 800 million pixels the full resolution mosaic strives to show all the stars the eye can see in planet Earth's night sky. Part of ESO's Gigagalaxy Zoom Project, the mosaicked images were recorded over several months of 2008 and 2009 at exceptional astronomical sites; the Atacama Desert in the southern hemisphere and the Canary Islands in the northern hemisphere. Also capturing bright planets and even a comet, the individual frames were stitched together and mapped into a single, flat, apparently seamless 360 by 180 degree view. The final result is oriented so the plane of our galaxy runs horizontally through the middle with the bulging Galactic Center at image center. Below and right of center are the Milky Way's satellite galaxies, the Magellanic Clouds.",https://apod.nasa.gov/apod/image/0909/milkywaypan_brunier_2048.jpg,image,v1,Gigagalaxy Zoom: Milky Way,https://apod.nasa.gov/apod/image/0909/milkywaypan_brunier_h600.jpg,Serge Brunier,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2013-03-11,"Why does a volcanic eruption sometimes create lightning? Pictured above, the Sakurajima volcano in southern Japan was caught erupting in early January. Magma bubbles so hot they glow shoot away as liquid rock bursts through the Earth's surface from below. The above image is particularly notable, however, for the lightning bolts caught near the volcano's summit. Why lightning occurs even in common thunderstorms remains a topic of research, and the cause of volcanic lightning is even less clear. Surely, lightning bolts help quench areas of opposite but separated electric charges. One hypothesis holds that catapulting magma bubbles or volcanic ash are themselves electrically charged, and by their motion create these separated areas. Other volcanic lightning episodes may be facilitated by charge-inducing collisions in volcanic dust. Lightning is usually occurring somewhere on Earth, typically over 40 times each second.",https://apod.nasa.gov/apod/image/1303/volcano_reitze_1280.jpg,image,v1,Sakurajima Volcano with Lightning,https://apod.nasa.gov/apod/image/1303/volcano_reitze_960.jpg," -Martin Rietze -(Alien Landscapes on Planet Earth) -",exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2019-04-22,"The methane mystery on Mars just got stranger. New results from ESA and Roscosmos' ExoMars Trace Gas Orbiter, has unexpectedly not detected methane in the atmosphere of Mars. This result follows the 2013 detection of methane by NASA's Curiosity rover, a result seemingly confirmed by ESA's orbiting Mars Express the next day. The issue is so interesting because life is a major producer of methane on Earth, leading to intriguing speculation that some sort of life -- possibly microbial life -- is creating methane beneath the surface of Mars. Non-biological sources of methane are also possible. Pictured is a visualization of the first claimed methane plume over Mars as detected from Earth in 2003. The new non-detection of methane by the ExoMars Orbiter could mean that Mars has some unexpected way of destroying methane, or that only some parts of Mars release methane -- and possibly only at certain times. As the mystery has now deepened, humanity's scrutiny of our neighboring planet's atmosphere will deepen as well.",,video,v1,Mars Methane Mystery Deepens,https://www.youtube.com/embed/rKBoYvVirwA?rel=0,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2006-05-21,"How can two stars create such a strange and intricate structure? Most stars are members of multiple-star systems. Some stars are members of close binary systems where material from one star swirls around the other in an accretion disk. Only a handful of stars, however, are members of an intermediate polar, a system featuring a white dwarf star with a magnetic field that significantly pushes out the inner accretion disk, only allowing material to fall down its magnetic poles. Shown above is an artist's depiction of an intermediate polar system, also known as a DQ Hercules system. The foreground white dwarf is so close to the normal star that it strips away its outer atmosphere. As the white dwarf spins, the columns of infalling gas rotate with it. The name intermediate polar derives from observations of emitted light polarized at a level intermediate to non-disk binary systems known as polars. Intermediate polars are a type of cataclysmic variable star system.",https://apod.nasa.gov/apod/image/0605/ipolar_garlick.jpg,image,v1,An Intermediate Polar Binary System,https://apod.nasa.gov/apod/image/0605/ipolar_garlick_big.jpg," -Mark Garlick -(Space-art) -",exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2002-11-24,"Why put observatories in space? Most telescopes are on the ground. On the ground, you can deploy a heavier telescope and fix it more easily. The trouble is that Earth-bound telescopes must look through the Earth's atmosphere. First, the Earth's atmosphere blocks out a broad range of the electromagnetic spectrum, allowing a narrow band of visible light to reach the surface. Telescopes which explore the Universe using light beyond the visible spectrum, such as those onboard the Chandra X-ray Observatory need to be carried above the absorbing atmosphere. Second, the Earth's atmosphere blurs the light it lets through. The blurring is caused by varying density and continual motion of air. By orbiting above the Earth's atmosphere, the Hubble Space Telescope, pictured above, can get clearer images. In fact, even though HST has a mirror 15 times smaller than large Earth-bound telescopes, it can still resolve finer details. A future large optical telescope in space is planned.",https://apod.nasa.gov/apod/image/0211/hst_sts82_big.jpg,image,v1,Hubble Floats Free,https://apod.nasa.gov/apod/image/0211/hst_sts82.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2017-02-11,"On Valentine's Day in 1990, cruising four billion miles from the Sun, the Voyager 1 spacecraft looked back one last time to make this first ever Solar System family portrait. The complete portrait is a 60 frame mosaic made from a vantage point 32 degrees above the ecliptic plane. In it, Voyager's wide angle camera frames sweep through the inner Solar System at the left, linking up with gas giant Neptune, the Solar System's outermost planet, at the far right. Positions for Venus, Earth, Jupiter, Saturn, Uranus, and Neptune are indicated by letters, while the Sun is the bright spot near the center of the circle of frames. The inset frames for each of the planets are from Voyager's narrow field camera. Unseen in the portrait are Mercury, too close to the Sun to be detected, and Mars, unfortunately hidden by sunlight scattered in the camera's optical system. Closer to the Sun than Neptune at the time, small, faint Pluto's position was not covered.",https://apod.nasa.gov/apod/image/1702/ssportrait_vg1_big.jpg,image,v1,Solar System Portrait,https://apod.nasa.gov/apod/image/1702/ssportrait_vg1.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -1997-04-03,"Does a comet's dust tail always orbit behind it? Since comets rotate, they shed gas and dust in all directions equally. Small ice and dust particles expelled by the comet, however, are literally pushed around by sunlight. The smaller the particle, the greater the effect. When the comet is headed inward, sunlight slows down small particles so they orbit behind the comet. When the comet is headed back out though, sunlight speeds them up, so small particles orbit in front of the comet. Comet Hale-Bopp itself is too big to have its orbit affected by the momentum of sunlight. Therefore, since Comet Hale-Bopp started back out to the outer Solar System two days ago, we can expect the dramatic dust tail shown above to shift in front in the coming days.",https://apod.nasa.gov/apod/image/9704/halebopp1_ja.jpg,image,v1,"Earth, Clouds, Sky, Comet -Credit and Copyright:",https://apod.nasa.gov/apod/image/9704/halebopp1_ja_big.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2003-07-08,"Nobody suspected that this volcano would erupt. Mt. Anatahan has not erupted in recorded history. Nevertheless, on May 10, the small volcano in the Northern Mariana Islands of the western Pacific Ocean shot ash 10,000 meters into the air. Explosions from Mt. Anatahan continued every few minutes for two days. The airborne ash was so bad that some flights were cancelled from downwind Guam. Although meter-sized rocks were catapulted through the air, nobody was hurt, as a seismology team that coincidentally installed detectors on the island a few days before had already left. Fortunately, the team was not too far away to get the above picture.",https://apod.nasa.gov/apod/image/0307/anatahanboom_sauter_big.jpg,image,v1,Mt. Anatahan Erupts,https://apod.nasa.gov/apod/image/0307/anatahanboom_sauter.jpg," -Allan Sauter -(Scripps) -",exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2020-02-01,"When leaving lunar orbit in February 1971, the crew of Apollo 14 watched this Earthrise from their command module Kitty Hawk. With Earth's sunlit crescent just peeking over the lunar horizon, the cratered terrain in the foreground is along the lunar farside. Of course, while orbiting the Moon, the crew could watch Earth rise and set, but the Earth hung stationary in the sky over Fra Mauro Base, their landing site on the lunar surface. Rock samples brought back by the Apollo 14 mission included a 20 pound rock nicknamed Big Bertha, later determined to contain a likely fragment of a meteorite from planet Earth.",https://apod.nasa.gov/apod/image/2002/AS14-71-9845v2wmktwtr4Jerry.jpg,image,v1,Apollo 14 Heads for Home,https://apod.nasa.gov/apod/image/2002/AS14-71-9845v2wmktwtr4Jerry1024.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2022-06-12,"Have you ever seen the Man in the Moon? This common question plays on the ability of humans to see pareidolia -- imagining familiar icons where they don't actually exist. The textured surface of Earth's full Moon is home to numerous identifications of iconic objects, not only in modern western culture but in world folklore throughout history. Examples, typically dependent on the Moon's perceived orientation, include the Woman in the Moon and the Rabbit in the Moon. One facial outline commonly identified as the Man in the Moon starts by imagining the two dark circular areas -- lunar maria -- here just above the Moon's center, to be the eyes. Surprisingly, there actually is a man in this Moon image -- a close look will reveal a real person -- with a telescope -- silhouetted against the Moon. This featured well-planned image was taken in 2016 in Cadalso de los Vidrios in Madrid, Spain. Do you have a favorite object that you see in the Moon?",https://apod.nasa.gov/apod/image/1602/ManInMoon_Caxete_2770.jpg,image,v1,Find the Man in the Moon,https://apod.nasa.gov/apod/image/1602/ManInMoon_Caxete_1080.jpg," -Dani Caxete -",exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2015-02-03,"Where do comet tails come from? Although it is common knowledge that comet tails and comas originate from comet nuclei, exactly how that happens is an active topic of research. One of the best images yet of emerging jets is shown in the featured image, taken last November by the robotic Rosetta spacecraft in orbit around the Comet 67P/Churyumov-Gerasimenko (Comet CG), and released last month. The overexposed picture shows plumes of gas and dust escaping numerous places from the Comet CG's nucleus as it nears the Sun and heats up. Although Comet CG is currently further out from the Sun than Mars, its orbit will take it almost as close as the Earth this coming August, at which time its jet activity is expected to increase by a factor of about 100. You've likely seen some debris from comet nuclei before but in another form -- when sand-sized bits end their journey through the Solar System by impacting the atmosphere of Earth as meteors. Almost Hyperspace: Random APOD Generator",https://apod.nasa.gov/apod/image/1502/CometPlumes_Rosetta_2048.jpg,image,v1,Jets from Comet Churyumov-Gerasimenko,https://apod.nasa.gov/apod/image/1502/CometPlumes_Rosetta_960.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2016-08-21,"Would you like to see a total eclipse of the Sun? If so, do any friends or relatives live near the path of next summer's eclipse? If yes again, then you might want to arrange a visit for one year from today. Next year on this exact date, the path of a total solar eclipse will cut right across the center of the contiguous USA. All of North America and part of South America will experience, at the least, a partial solar eclipse. Featured here is a map of the path of totality, computed by eclipse expert Fred Espenak of NASA's GSFC. Many people who have seen a total solar eclipse tell stories about it for the rest of their lives. The last path of solar totality that included any part of the contiguous USA was in 1979, and the next two will be in 2024 and 2044. Zoom in: An interactive map of the eclipse path.",https://apod.nasa.gov/apod/image/1608/TSE2017usa_espenak_1421.jpg,image,v1,Map of Total Solar Eclipse Path in 2017 August,https://apod.nasa.gov/apod/image/1608/TSE2017usa_espenak_1080.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2003-04-11,"Do you recognize this intriguing globular cluster of stars? It's actually the constellation of city lights surrounding London, England, planet Earth, as recorded with a digital camera from the International Space Station. Taken in February 2003, north is toward the top and slightly left in this nighttime view. The encircling ""London Orbital"" highway by-pass, the M25 (... but not Messier 25), is easiest to pick out south of the city. Even farther south are the lights of Gatwick airport and just inside the western (left hand) stretch of the Orbital is Heathrow. The darkened Thames river estuary fans out to the city's east. In particular, two small ""dark nebulae"" - Hyde Park and Regents Park - stand out slightly west of the densely packed lights at the city's core. Have you seen this: NASA Image of the Day?",https://apod.nasa.gov/apod/image/0304/london_iss_full.jpg,image,v1,London at Night,https://apod.nasa.gov/apod/image/0304/london_iss_c1.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2017-11-13,"Why is Comet Maccholz so depleted of carbon-containing chemicals? Comet 96P/Machholz's original fame derives from its getting closer to the Sun than any other short period comet -- half as close as Mercury -- and doing so every five years. To better understand this unusual comet, NASA's Sun-monitoring SOHO spacecraft tracked the comet during its latest approach to the Sun in October. The featured image composite shows the tail-enhanced comet swooping past the Sun. The Sun's bright surface is hidden from view behind a dark occulter, although parts of the Sun's extended corona are visible. Neighboring stars dot the background. One hypothesis holds that these close solar approaches somehow cause Comet Machholz to shed its carbon, while another hypothesis posits that the comet formed with this composition far away -- possibly even in another star system. Free APOD Lectures: January 5 in NYC & January 9 in DC",https://apod.nasa.gov/apod/image/1711/CometMachholz2017_SOHO_big.mp4,image,v1,Comet Machholz Approaches the Sun,https://apod.nasa.gov/apod/image/1711/CometMachholz2017_SOHO_960.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2000-03-27,"What would it look like to fly over an asteroid? Spacecraft NEAR Shoemaker in orbit around asteroid 433 Eros found out earlier this month when it recorded its first fly-over sequence. The saddle region of the Sun-orbiting space-mountain appears to zip past the camera in this condensed hour-long time-lapse sequence. The spacecraft was orbiting about 200 kilometers above the asteroid. Movies such as this are scientifically useful for discerning between regions that are naturally dark and regions that have their brightness dominated by shadows. The week before, a bright X-ray burst from the Sun allowed NEAR's X-ray spectrometer to detect the presence of several elements on Eros' surface by their X-ray fluorescent signatures.",https://apod.nasa.gov/apod/image/0003/flyover1_near.gif,image,v1,Flying Over Asteroid Eros,https://apod.nasa.gov/apod/image/0003/flyover1_near_big.gif,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2013-07-12,"This fifteen degree wide field of view stretches across the crowded starfields of Sagittarius toward the center of our Milky Way galaxy. In fact, the center of the galaxy lies near the right edge of the rich starscape and eleven bright star clusters and nebulae fall near the center of the frame. All eleven are numbered entries in the catalog compiled by 18th century cosmic tourist Charles Messier. Gaining celebrity status with skygazers, M8 (Lagoon), M16 (Eagle), M17 (Omega), and M20 (Trifid) show off the telltale reddish hues of emission nebulae associated with star forming regions. But also eye-catching in small telescopes are star clusters in the crowded region; M18, M21, M22, M23, M25, and M28. Broader in extent than the star clusters themselves, M24 is actually a cloud of the Milky Way's stars thousands of light-years long, seen through a break in the galaxy's veil of obscuring dust. You can put your cursor over the image (or click here) for help identifying Messier's eleven.",https://apod.nasa.gov/apod/image/1307/20130706_elevenMessiers.jpg,image,v1,Messier's Eleven,https://apod.nasa.gov/apod/image/1307/20130706_elevenMessiers950.jpg,Fernando Cabrerizo,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2018-04-17,"cept for the rings of Saturn, the Ring Nebula (M57) is probably the most famous celestial band. Its classic appearance is understood to be due to our own perspective, though. The recent mapping of the expanding nebula's 3-D structure, based in part on this clear Hubble image,indicates that the nebula is a relatively dense, donut-like ring wrapped around the middle of a (American) football-shaped cloud of glowing gas. The view from planet Earth looks down the long axis of the football, face-on to the ring. Of course, in this well-studied example of a planetary nebula, the glowing material does not come from planets. Instead, the gaseous shroud represents outer layers expelled from the dying, once sun-like star, now a tiny pinprick of light seen at the nebula's center. Intense ultraviolet light from the hot central star ionizes atoms in the gas. The Ring Nebula is about one light-year across and 2,000 light-years away. Share the Sky: NASA Open API for APOD",https://apod.nasa.gov/apod/image/1804/Ring_HubbleDonatiello_3251.jpg,image,v1,M57: The Ring Nebula,https://apod.nasa.gov/apod/image/1804/Ring_HubbleDonatiello_960.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2011-02-21,"What's visible in the night sky during this time of year? To help illustrate the answer, a beautiful land, cloud, and skyscape was captured earlier this month over Neuch�tel, Switzerland. Visible in the foreground were the snow covered cliffs of the amphitheater shaped Creux du Van, as well as distant trees, and town-lit clouds. Visible in the night sky (at midnight) were galaxies including the long arch of the central band of our Milky Way Galaxy, the Andromeda galaxy (M31), and the Triangulum galaxy (M33). Star clusters visible included NGC 752, M34, M35, M41, the double cluster, and the Beehive (M44). Nebulas visible included the Orion Nebula (M42), NGC 7822, IC 1396, the Rosette Nebula, the Flaming Star Nebula, the California Nebula, the Heart and Soul Nebulas, and the Pacman Nebula. Rolling your cursor over the above image will bring up labels for all of these. But the above wide angle sky image captured even more sky wonders. What other nebulas can you find in the above image?",https://apod.nasa.gov/apod/image/1102/mwcliffs_vetter_2000.jpg,image,v1,Milky Way Over Switzerland,https://apod.nasa.gov/apod/image/1102/mwcliffs_vetter_900.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2016-12-17,"Southern Jupiter looms some 37,000 kilometers away in this JunoCam image from December 11. The image data was captured near Juno's third perijove or closest approach to Jupiter, the spacecraft still in its 53 day long looping orbit. With the south polar region on the left, the large whitish oval toward the right is massive, counterclockwise rotating storm system. Smaller than the more famous Great Red Spot, the oval storm is only about half the diameter of planet Earth, one of a string of white ovals currently in the southern hemisphere of the Solar System's, ruling gas giant.",https://apod.nasa.gov/apod/image/1612/2016-12-11T173502JunoPerijove3Peach.jpg,image,v1,Southern Jupiter from Perijove 3,https://apod.nasa.gov/apod/image/1612/2016-12-11T173502JunoPerijove3Peach1024.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2007-05-11,"The silhouette of an intriguing dark nebula inhabits this cosmic scene, based on images from the Palomar Observatory Sky Survey. Lynds' Dark Nebula (LDN) 1622 appears against a faint background of glowing hydrogen gas only easily seen in long telescopic exposures of the region. LDN 1622 lies near the plane of our Milky Way Galaxy, close on the sky to Barnard's Loop - a large cloud surrounding the rich complex of emission nebulae found in the Belt and Sword of Orion. But the obscuring dust of LDN 1622 is thought to be much closer than Orion's more famous nebulae, perhaps only 500 light-years away. At that distance, this 1 degree wide field of view would span less than 10 light-years.",https://apod.nasa.gov/apod/image/0705/ldn1622_carboni.jpg,image,v1,LDN 1622: Dark Nebula in Orion,https://apod.nasa.gov/apod/image/0705/ldn1622_carboni_c720.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2020-02-07,"Big, beautiful spiral galaxy NGC 7331 is often touted as an analog to our own Milky Way. About 50 million light-years distant in the northern constellation Pegasus, NGC 7331 was recognized early on as a spiral nebula and is actually one of the brighter galaxies not included in Charles Messier's famous 18th century catalog. Since the galaxy's disk is inclined to our line-of-sight, long telescopic exposures often result in an image that evokes a strong sense of depth. This Hubble Space Telescope close-up spans some 40,000 light-years. The galaxy's magnificent spiral arms feature dark obscuring dust lanes, bright bluish clusters of massive young stars, and the telltale reddish glow of active star forming regions. The bright yellowish central regions harbor populations of older, cooler stars. Like the Milky Way, a supermassive black hole lies at the core of spiral galaxy NGC 7331.",https://apod.nasa.gov/apod/image/2002/potw1805a_ngc7331.jpg,image,v1,NGC 7331 Close Up,https://apod.nasa.gov/apod/image/2002/potw1805b_ngc7331.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2017-11-18,"Friday, an old Moon smiled for early morning risers. Its waning sunlit crescent is captured in this atmospheric scene from clear skies near Bursa, Turkey, planet Earth. In the subtle twilight hues nearby celestial lights are Jupiter (top) and Venus shining close to the eastern horizon. But today, Saturday, the Moon will be new and early next week its waxing crescent will follow the setting Sun as it sinks in the west. Then, a young Moon's smile will join Saturn and Mercury in early evening skies. Watch: Leonid Meteor Shower",https://apod.nasa.gov/apod/image/1711/20171117dawnTezel.jpg,image,v1,"Friday, the Moon Smiled",https://apod.nasa.gov/apod/image/1711/20171117dawnTezel1200c.jpg,Tunç Tezel,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2003-02-14,"Yes, it's Valentine's Day (!) and looking toward star cluster NGC 346 in our neighboring galaxy the Small Magellanic Cloud, astronomers have noted this heart-shaped cloud of hot, x-ray emitting gas in the cluster's central region. The false-color Chandra Observatory x-ray image also shows a strong x-ray source just above the heart-shaped cloud which corresponds to HD 5980, a remarkable, massive binary star system that lies within the cluster. HD 5980 has been known to undergo dramatic brightness variations, in 1994 briefly outshining all other stars in the Small Magellanic Cloud, and has been likened to the luminous, eruptive variable star Eta Carinae in our own Milky Way galaxy. At about 100 light-years across, NGC 346's heart-shaped cloud is probably the result of an ancient supernova explosion. Alternatively it may have been produced during past eruptions from the HD 5980 system, analogous to the nebula associated with Eta Carinae.",https://apod.nasa.gov/apod/image/0302/ngc346_cxo_full.jpg,image,v1,The Heart in NGC 346,https://apod.nasa.gov/apod/image/0302/ngc346_cxo_c1.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -1998-06-20,"Q: What was made by humans and is 6.5 billion miles away? A: Pioneer 10 - and last year was the 25th anniversary of its launch. More than 9.5 light-hours distant, Pioneer 10 is presently about twice as far from the Sun as Pluto, bound for interstellar space at 28,000 miles per hour. The distinction of being the first human artifact to venture beyond the Solar System is just one in a long list of firsts for this spacefaring ambassador, including; the first spacecraft to travel through the asteroid belt and explore the outer Solar System, the first spacecraft to visit Jupiter, the first to use a planet's gravity to change its course and to reach solar-system-escape velocity, and the first spacecraft to pass beyond the known planets. Pioneer 10's mission is nearing an end - now exploring the distant reaches of the heliosphere it will soon run out of sufficient electrical power to operate science instruments. However, the 570 lb. spacecraft will continue to coast and in 30,000 years or so it will pass within about 3 light years of a nearby star known as Ross 248. Ross 248 is a faint red dwarf just over 10 light years distant in the constellation Taurus. (Note: This year Voyager 1, launched 21 years ago but traveling faster than Pioneer 10, became humanity's most distant spacecraft.)",https://apod.nasa.gov/apod/image/9703/pioneer10_art.jpg,image,v1,Pioneer 10: The First 6 Billion Miles,https://apod.nasa.gov/apod/image/9703/pioneer10_art.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2017-07-02,"It's stars versus dust in the Carina Nebula and the stars are winning. More precisely, the energetic light and winds from massive newly formed stars are evaporating and dispersing the dusty stellar nurseries in which they formed. Located in the Carina Nebula and known informally as Mystic Mountain, these pillar's appearance is dominated by the dark dust even though it is composed mostly of clear hydrogen gas. Dust pillars such as these are actually much thinner than air and only appear as mountains due to relatively small amounts of opaque interstellar dust. About 7,500 light-years distant, the featured image was taken with the Hubble Space Telescope and highlights an interior region of Carina which spans about three light years. Within a few million years, the stars will likely win out completely and the entire dust mountain will evaporate.",https://apod.nasa.gov/apod/image/1707/carina08_hubble_2104.jpg,image,v1,Mountains of Dust in the Carina Nebula,https://apod.nasa.gov/apod/image/1707/carina08_hubble_960.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2014-01-05,"What's happening to galaxy NGC 474? The multiple layers of emission appear strangely complex and unexpected given the relatively featureless appearance of the elliptical galaxy in less deep images. The cause of the shells is currently unknown, but possibly tidal tails related to debris left over from absorbing numerous small galaxies in the past billion years. Alternatively the shells may be like ripples in a pond, where the ongoing collision with the spiral galaxy just above NGC 474 is causing density waves to ripple though the galactic giant. Regardless of the actual cause, the above image dramatically highlights the increasing consensus that at least some elliptical galaxies have formed in the recent past, and that the outer halos of most large galaxies are not really smooth but have complexities induced by frequent interactions with -- and accretions of -- smaller nearby galaxies. The halo of our own Milky Way Galaxy is one example of such unexpected complexity. NGC 474 spans about 250,000 light years and lies about 100 million light years distant toward the constellation of the Fish (Pisces). News: Follow APOD on Instagram.",https://apod.nasa.gov/apod/image/1401/ngc474_cfht_1769.jpg,image,v1,Galaxy NGC 474: Shells and Star Streams,https://apod.nasa.gov/apod/image/1401/ngc474_cfht_960.jpg," -P.-A. Duc -(CEA, -CFHT), -Atlas 3D Collaboration -",exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2020-07-27,"Normally, Steamboat Point looks cool -- but not this cool. Every day, the iconic peak of the Bighorn Mountains is an interesting sight, in particular from US Highway 14 in Wyoming. On some rare days, the rocky vertical ridges look even more incredible when seen in front of a distant lightning storm. Earlier this month, though, something even more unusual happened -- the naked-eye Comet NEOWISE rose above it in the middle of the night. Just as a distant lightning storm was occurring in the background. Recognizing a rare opportunity, a determined astrophotographer spent a sleepless night capturing over 1400 images of this unusual triple conjunction. The featured image is among the best of them, with the foreground lit by the Moon off to the right. Comet C/2020 F3 (NEOWISE) is now headed back to the outer Solar System, destined to return only in about 6700 years. Comet NEOWISE Images: July 26 || 25 || 24 || 23 || 22 || 21 || 20 || 19 || 18 || 17 || 16 || 15 || 14 || 13 || 12 || 11 || 10 & earlier ||",https://apod.nasa.gov/apod/image/2007/CometLightning_Palmer_1920.jpg,image,v1,Comet and Lightning Beyond Bighorn Mountains,https://apod.nasa.gov/apod/image/2007/CometLightning_Palmer_960.jpg," -Kevin Palmer -",exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2022-04-25,"In one of the brightest parts of Milky Way lies a nebula where some of the oddest things occur. NGC 3372, known as the Great Nebula in Carina, is home to massive stars and changing nebulas. The Keyhole Nebula (NGC 3324), the bright structure just below the image center, houses several of these massive stars. The entire Carina Nebula, captured here, spans over 300 light years and lies about 7,500 light-years away in the constellation of Carina. Eta Carinae, the most energetic star in the nebula, was one of the brightest stars in the sky in the 1830s, but then faded dramatically. While Eta Carinae itself maybe on the verge of a supernova explosion, X-ray images indicate that much of the Great Nebula in Carina has been a veritable supernova factory.",https://apod.nasa.gov/apod/image/2204/CarinaMosaic_Bobillo_1600.jpg,image,v1,The Great Nebula in Carina,https://apod.nasa.gov/apod/image/2204/CarinaMosaic_Bobillo_960.jpg," -Ignacio Javier Diaz Bobillo -",exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2014-07-29,"To some, it may look like a portal into the distant universe. To others, it may appear as the eye of a giant. Given poetic license, both are correct. Pictured above is a standard fisheye view of the sky -- but with an unusual projection. The view is from a perch in New Zealand called Te Mata Peak, a name that translates from the Maori language as ""Sleeping Giant"". The wondrous panorama shows the band of our Milky Way Galaxy right down the center of the sky, with the Large and Small Magellanic Clouds visible to the right. The red hue is atmospheric airglow that surprised the photographer as it was better captured by the camera than the eye. The above image was taken two weeks ago as the photographer's sister, on the left, and an acquaintance peered into the sky portal.",https://apod.nasa.gov/apod/image/1407/SkyPortal_horalek_1500.jpg,image,v1,A Sky Portal in New Zealand,https://apod.nasa.gov/apod/image/1407/SkyPortal_horalek_960.jpg," -Petr Hor�lek -",exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2003-11-28,"A false-color x-ray image inset at upper left reveals emission from a cosmic jet of high-energy particles, 100,000 light-years in length, emerging from quasar GB1508+5714. An estimated 12 billion (12,000,000,000) light-years away, this appears to be the most distant energetic jet in the known Universe. Astrophysical jets of many sizes seem to be produced in a range of environments where significant accretion, or infalling matter is thought to arrange itself in a disk, from contracting star-forming clouds to supermassive black holes in active galactic nuclei. Here, as depicted in the illustration, the accretion disk is thought to surround a supermassive black hole, accelerating particles to near the speed of light in two jets at right angles to the disk itself. In the case of this quasar, the jet tilted towards us is visible in x-rays as the particles collide with low energy photons from the cosmic background radiation. The collisions boost the photons to higher x-ray energies and scatter some of them in our direction.",https://apod.nasa.gov/apod/image/0311/gb1508_xray_illustration.jpg,image,v1,The Most Distant X-Ray Jet,https://apod.nasa.gov/apod/image/0311/gb1508_xray_illustration90.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2013-10-10,"Interstellar dust clouds and bright nebulae abound in the fertile constellation of Orion. One of the brightest, M78, is just left of center in this colorful telescopic view, covering an area north of Orion's belt. At a distance of about 1,500 light-years, the bluish nebula itself is about 5 light-years across. Its blue tint is due to dust preferentially reflecting the blue light of hot, young stars in the region. Dark dust lanes and other nebulae can easily be traced through this gorgeous skyscape. The scene also includes the remarkable McNeil's Nebula -- a newly recognized nebula associated with the formation of a sun-like star, and the telltale reddish glow of many Herbig- Haro objects, energetic jets from stars in the process of formation. Note: How to find APOD Alternative Mirror Sites",https://apod.nasa.gov/apod/image/1310/M78_hallas.jpg,image,v1,M78: Stardust and Starlight,https://apod.nasa.gov/apod/image/1310/M78_hallas950.jpg,Tony Hallas,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2014-08-09,"What shines in the world at night? Just visible to the eye, a rare electric blue glow spread along the shores of Victoria Lake on January 16, 2013. Against reflections of a light near the horizon, this digitally stacked long exposure recorded the bioluminescence of Noctiluca scintillans, plankton stimulated by the lapping waves. Above, the night skies of the Gippsland Lakes region, Victoria, Australia shine with a fainter greenish airglow. Oxygen atoms in the upper atmosphere, initially excited by ultraviolet sunlight, produce the more widely seen fading atmospheric chemiluminescence. Washed out by the Earth's rotation, the faint band of the southern summer Milky Way stretches from the horizon as star trails circle the South Celestial Pole. Watch: Meteors vs. Supermoon",https://apod.nasa.gov/apod/image/1408/BioluminescenceMW_PhilHart.jpg,image,v1,A Luminous Night,https://apod.nasa.gov/apod/image/1408/BioluminescenceMW_PhilHart1024.jpg,Phil Hart,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -1997-12-01,"Orion is big. Some of the stars that form the constellation of Orion are part of a giant gas cloud complex that stretches over 100 light years and appears more than 50 times the diameter of the Moon. Components of this cloud include the Horsehead Nebula, the Orion Nebula, the Trapezium open cluster, and small disks containing stellar systems which are just forming. At 1500 light years, Orion is the closest star forming region to Earth. Close inspection of the photo's center should reveal the three stars which form the belt of Orion.",https://apod.nasa.gov/apod/image/9712/orionfull_jcc_big.jpg,image,v1,Orion: The Big Picture,https://apod.nasa.gov/apod/image/9712/orionfull_jcc.jpg," -J. C. Casado -",exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2018-09-12,"Our Moon's appearance changes nightly. As the Moon orbits the Earth, the half illuminated by the Sun first becomes increasingly visible, then decreasingly visible. The featured video animates images taken by NASA's Moon-orbiting Lunar Reconnaissance Orbiter to show all 12 lunations that appear this year, 2018. A single lunation describes one full cycle of our Moon, including all of its phases. A full lunation takes about 29.5 days, just under a month (moon-th). As each lunation progresses, sunlight reflects from the Moon at different angles, and so illuminates different features differently. During all of this, of course, the Moon always keeps the same face toward the Earth. What is less apparent night-to-night is that the Moon's apparent size changes slightly, and that a slight wobble called a libration occurs as the Moon progresses along its elliptical orbit.",,video,v1,Lunations,https://www.youtube.com/embed/5Om7NbfUC6Y?rel=0,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2001-10-31,"Halloween's origin is ancient and astronomical. Since the fifth century BC, Halloween has been celebrated as a cross-quarter day, a day halfway between an equinox (equal day / equal night) and a solstice (minimum day / maximum night in the northern hemisphere). With our modern calendar, however, the real cross-quarter day will occur next week. Another cross-quarter day is Groundhog's Day. Halloween's modern celebration retains historic roots in dressing to scare away the spirits of the dead. A perhaps-fitting modern tribute to this ancient holiday is the above-pictured Ghost Head Nebula taken with the Hubble Space Telescope. Appearing similar to the icon of a fictional ghost, NGC 2080 is actually a star forming region in the Large Magellanic Cloud, a satellite galaxy of our own Milky Way Galaxy. The Ghost Head Nebula spans about 50 light-years and is shown in representative colors.",https://apod.nasa.gov/apod/image/0110/ngc2080_hst_big.jpg,image,v1,Halloween and the Ghost Head Nebula,https://apod.nasa.gov/apod/image/0110/ngc2080_hst.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -2013-04-11,"In a haunting vista you can never see, bright stars and the central Milky Way rise over the dark skyline of metropolitan Pudong in Shanghai, China. Looking east across the Huangpu River, the cityscape includes Pudong's 470 meter tall Oriental Pearl Tower. The night sky stretches from Antares and the stars of Scorpius at the far right, to Altair in Aquila at the left. To create the vision of an unseen reality, part of a series of Darkened Cities, photographer Thierry Cohen has combined a daytime image of the city skyline with an image matched in orientation from a dark sky region at the same latitude, just west of Merzouga, Morocco. The result finds the night sky that hours earlier also arced over Shanghai, but drowned in the lights of a city upon the sea.",https://apod.nasa.gov/apod/image/1304/ShanghaiPudongDCThierryCohen900.jpg,image,v1,Darkened City,https://apod.nasa.gov/apod/image/1304/ShanghaiPudongDCThierryCohen900.jpg,Photo Thierry Cohen,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:37:13.715250 -,,,,,,,,star,{'self': 'http://api.nasa.gov/neo/rest/v1/neo/2000433?api_key=PBI6QS2eOkQigQpGPHNNCTxvPbSzakdW2Nq8R7yS'},2000433,2000433,433 Eros (A898 PA),Eros,433,https://ssd.jpl.nasa.gov/tools/sbdb_lookup.html#/?sstr=2000433,10.41,"{'kilometers': {'estimated_diameter_min': 22.0067027115, 'estimated_diameter_max': 49.2084832235}, 'meters': {'estimated_diameter_min': 22006.7027114738, 'estimated_diameter_max': 49208.4832234845}, 'miles': {'estimated_diameter_min': 13.6743268705, 'estimated_diameter_max': 30.5767244291}, 'feet': {'estimated_diameter_min': 72200.4705239119, 'estimated_diameter_max': 161445.1600989368}}",False,"[{'close_approach_date': '1900-12-27', 'close_approach_date_full': '1900-Dec-27 01:30', 'epoch_date_close_approach': -2177879400000, 'relative_velocity': {'kilometers_per_second': '5.5786191875', 'kilometers_per_hour': '20083.0290749201', 'miles_per_hour': '12478.8132604691'}, 'miss_distance': {'astronomical': '0.3149291693', 'lunar': '122.5074468577', 'kilometers': '47112732.928149391', 'miles': '29274494.7651919558'}, 'orbiting_body': 'Earth'}, {'close_approach_date': '1907-11-05', 'close_approach_date_full': '1907-Nov-05 03:31', 'epoch_date_close_approach': -1961526540000, 'relative_velocity': {'kilometers_per_second': '4.3944908885', 'kilometers_per_hour': '15820.1671985367', 'miles_per_hour': '9830.0366684463'}, 'miss_distance': {'astronomical': '0.4714855425', 'lunar': '183.4078760325', 'kilometers': '70533232.893794475', 'miles': '43827318.620434755'}, 'orbiting_body': 'Earth'}, {'close_approach_date': '1917-04-20', 'close_approach_date_full': 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'kilometers': '39833635.134625859', 'miles': '24751473.1315964942'}, 'orbiting_body': 'Earth'}, {'close_approach_date': '1975-01-23', 'close_approach_date_full': '1975-Jan-23 07:39', 'epoch_date_close_approach': 159694740000, 'relative_velocity': {'kilometers_per_second': '5.8253076833', 'kilometers_per_hour': '20971.1076598791', 'miles_per_hour': '13030.6307567732'}, 'miss_distance': {'astronomical': '0.1511341909', 'lunar': '58.7912002601', 'kilometers': '22609353.042813383', 'miles': '14048800.5292673654'}, 'orbiting_body': 'Earth'}, {'close_approach_date': '1981-12-29', 'close_approach_date_full': '1981-Dec-29 08:05', 'epoch_date_close_approach': 378461100000, 'relative_velocity': {'kilometers_per_second': '5.6652718459', 'kilometers_per_hour': '20394.9786453535', 'miles_per_hour': '12672.6465921642'}, 'miss_distance': {'astronomical': '0.3084893271', 'lunar': '120.0023482419', 'kilometers': '46149346.251893277', 'miles': '28675874.0429781426'}, 'orbiting_body': 'Earth'}, {'close_approach_date': '1988-11-06', 'close_approach_date_full': '1988-Nov-06 14:56', 'epoch_date_close_approach': 594831360000, 'relative_velocity': {'kilometers_per_second': '4.305902138', 'kilometers_per_hour': '15501.2476969045', 'miles_per_hour': '9631.8724925571'}, 'miss_distance': {'astronomical': '0.4676402077', 'lunar': '181.9120407953', 'kilometers': '69957978.998277599', 'miles': '43469872.4247609062'}, 'orbiting_body': 'Earth'}, {'close_approach_date': '2005-03-08', 'close_approach_date_full': '2005-Mar-08 22:07', 'epoch_date_close_approach': 1110319620000, 'relative_velocity': {'kilometers_per_second': '4.4122923953', 'kilometers_per_hour': '15884.2526231559', 'miles_per_hour': '9869.8568590937'}, 'miss_distance': {'astronomical': '0.3655672222', 'lunar': '142.2056494358', 'kilometers': '54688077.782936714', 'miles': '33981595.7867820932'}, 'orbiting_body': 'Earth'}, {'close_approach_date': '2012-01-31', 'close_approach_date_full': '2012-Jan-31 11:01', 'epoch_date_close_approach': 1328007660000, 'relative_velocity': {'kilometers_per_second': '5.9451959021', 'kilometers_per_hour': '21402.705247412', 'miles_per_hour': '13298.8087133156'}, 'miss_distance': {'astronomical': '0.1786758136', 'lunar': '69.5048914904', 'kilometers': '26729521.135077032', 'miles': '16608954.2658937616'}, 'orbiting_body': 'Earth'}, {'close_approach_date': '2019-01-15', 'close_approach_date_full': '2019-Jan-15 06:01', 'epoch_date_close_approach': 1547532060000, 'relative_velocity': {'kilometers_per_second': '6.0449176185', 'kilometers_per_hour': '21761.7034264303', 'miles_per_hour': '13521.8762207172'}, 'miss_distance': {'astronomical': '0.2085986871', 'lunar': '81.1448892819', 'kilometers': '31205919.274956477', 'miles': '19390459.0899223026'}, 'orbiting_body': 'Earth'}, {'close_approach_date': '2025-11-30', 'close_approach_date_full': '2025-Nov-30 02:18', 'epoch_date_close_approach': 1764469080000, 'relative_velocity': {'kilometers_per_second': 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'miss_distance': {'astronomical': '0.2725553389', 'lunar': '106.0240268321', 'kilometers': '40773698.156568143', 'miles': '25335601.2070526534'}, 'orbiting_body': 'Earth'}, {'close_approach_date': '2056-01-24', 'close_approach_date_full': '2056-Jan-24 11:03', 'epoch_date_close_approach': 2715937380000, 'relative_velocity': {'kilometers_per_second': '5.8207578574', 'kilometers_per_hour': '20954.7282866821', 'miles_per_hour': '13020.4532512442'}, 'miss_distance': {'astronomical': '0.1497821765', 'lunar': '58.2652666585', 'kilometers': '22407094.568364055', 'miles': '13923122.940991759'}, 'orbiting_body': 'Earth'}, {'close_approach_date': '2062-12-31', 'close_approach_date_full': '2062-Dec-31 08:25', 'epoch_date_close_approach': 2934779100000, 'relative_velocity': {'kilometers_per_second': '5.7322434825', 'kilometers_per_hour': '20636.0765370681', 'miles_per_hour': '12822.4554460466'}, 'miss_distance': {'astronomical': '0.3029535232', 'lunar': '117.8489205248', 'kilometers': '45321201.779715584', 'miles': '28161288.9295956992'}, 'orbiting_body': 'Earth'}, {'close_approach_date': '2069-11-08', 'close_approach_date_full': '2069-Nov-08 21:29', 'epoch_date_close_approach': 3151171740000, 'relative_velocity': {'kilometers_per_second': '4.2454176851', 'kilometers_per_hour': '15283.5036662481', 'miles_per_hour': '9496.5748197307'}, 'miss_distance': {'astronomical': '0.4647282185', 'lunar': '180.7792769965', 'kilometers': '69522351.616494595', 'miles': '43199186.121611611'}, 'orbiting_body': 'Earth'}, {'close_approach_date': '2086-03-11', 'close_approach_date_full': '2086-Mar-11 22:55', 'epoch_date_close_approach': 3666725700000, 'relative_velocity': {'kilometers_per_second': '4.2258643769', 'kilometers_per_hour': '15213.1117567663', 'miles_per_hour': '9452.8360246418'}, 'miss_distance': {'astronomical': '0.3713100271', 'lunar': '144.4396005419', 'kilometers': '55547189.163802277', 'miles': '34515422.8449623426'}, 'orbiting_body': 'Earth'}, {'close_approach_date': 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{'kilometers_per_second': '4.185536687', 'kilometers_per_hour': '15067.9320731868', 'miles_per_hour': '9362.6270151421'}, 'miss_distance': {'astronomical': '0.4511330659', 'lunar': '175.4907626351', 'kilometers': '67488545.745209633', 'miles': '41935437.7539856154'}, 'orbiting_body': 'Earth'}, {'close_approach_date': '2180-02-23', 'close_approach_date_full': '2180-Feb-23 19:43', 'epoch_date_close_approach': 6631616580000, 'relative_velocity': {'kilometers_per_second': '3.671684452', 'kilometers_per_hour': '13218.06402717', 'miles_per_hour': '8213.1909506602'}, 'miss_distance': {'astronomical': '0.4035358886', 'lunar': '156.9754606654', 'kilometers': '60368109.403117282', 'miles': '37511003.7747392116'}, 'orbiting_body': 'Earth'}, {'close_approach_date': '2180-06-16', 'close_approach_date_full': '2180-Jun-16 03:59', 'epoch_date_close_approach': 6641409540000, 'relative_velocity': {'kilometers_per_second': '13.4145453162', 'kilometers_per_hour': '48292.363138298', 'miles_per_hour': '30006.9964177941'}, 'miss_distance': {'astronomical': '0.3669611826', 'lunar': '142.7479000314', 'kilometers': '54896611.289641062', 'miles': '34111172.4992961756'}, 'orbiting_body': 'Earth'}, {'close_approach_date': '2192-06-06', 'close_approach_date_full': '2192-Jun-06 01:59', 'epoch_date_close_approach': 7019229540000, 'relative_velocity': {'kilometers_per_second': '9.0785215085', 'kilometers_per_hour': '32682.6774304402', 'miles_per_hour': '20307.7447622644'}, 'miss_distance': {'astronomical': '0.203838334', 'lunar': '79.293111926', 'kilometers': '30493780.59074858', 'miles': '18947956.630667204'}, 'orbiting_body': 'Earth'}]","{'orbit_id': '775', 'orbit_determination_date': '2024-04-11 06:19:11', 'first_observation_date': '1973-03-10', 'last_observation_date': '2024-04-10', 'data_arc_in_days': 18659, 'observations_used': 5761, 'orbit_uncertainty': '0', 'minimum_orbit_intersection': '.0637451', 'jupiter_tisserand_invariant': '4.640', 'epoch_osculation': '2460600.5', 'eccentricity': '.2561211105938557', 'semi_major_axis': '1.430429373177625', 'inclination': '8.708662579039903', 'ascending_node_longitude': '246.2950687062965', 'orbital_period': '624.8820596015659', 'perihelion_distance': '1.064066213493299', 'perihelion_argument': '338.4561585752549', 'aphelion_distance': '1.796792532861952', 'perihelion_time': '2460548.592807355109', 'mean_anomaly': '29.90418602204014', 'mean_motion': '.5761087143861058', 'equinox': 'J2000', 'orbit_class': {'orbit_class_type': 'AMO', 'orbit_class_description': 'Near-Earth asteroid orbits similar to that of 1221 Amor', 'orbit_class_range': '1.017 AU < q (perihelion) < 1.3 AU'}}",False,NASA,2024-12-20 19:37:13.715250 -,,,,,,,,star,{'self': 'http://api.nasa.gov/neo/rest/v1/neo/2001980?api_key=PBI6QS2eOkQigQpGPHNNCTxvPbSzakdW2Nq8R7yS'},2001980,2001980,1980 Tezcatlipoca (1950 LA),Tezcatlipoca,1980,https://ssd.jpl.nasa.gov/tools/sbdb_lookup.html#/?sstr=2001980,13.83,"{'kilometers': {'estimated_diameter_min': 4.5556985234, 'estimated_diameter_max': 10.1868515832}, 'meters': {'estimated_diameter_min': 4555.6985233574, 'estimated_diameter_max': 10186.8515832225}, 'miles': {'estimated_diameter_min': 2.8307789472, 'estimated_diameter_max': 6.3298141551}, 'feet': {'estimated_diameter_min': 14946.5179433719, 'estimated_diameter_max': 33421.4301482999}}",False,[],"{'orbit_id': '854', 'orbit_determination_date': '2024-12-19 05:31:50', 'first_observation_date': '1950-06-19', 'last_observation_date': '2024-12-18', 'data_arc_in_days': 27211, 'observations_used': 7813, 'orbit_uncertainty': '0', 'minimum_orbit_intersection': '.245309', 'jupiter_tisserand_invariant': '3.996', 'epoch_osculation': '2460600.5', 'eccentricity': '.3646719380908604', 'semi_major_axis': '1.709652145917187', 'inclination': '26.87082083094132', 'ascending_node_longitude': '246.5449690574104', 'orbital_period': '816.5072784800496', 'perihelion_distance': '1.086189984404368', 'perihelion_argument': '115.5094132367951', 'aphelion_distance': '2.333114307430006', 'perihelion_time': '2460520.990030834066', 'mean_anomaly': '35.05613440828088', 'mean_motion': '.440902377098401', 'equinox': 'J2000', 'orbit_class': {'orbit_class_type': 'AMO', 'orbit_class_description': 'Near-Earth asteroid orbits similar to that of 1221 Amor', 'orbit_class_range': '1.017 AU < q (perihelion) < 1.3 AU'}}",False,NASA,2024-12-20 19:37:13.715250 +Credit:",https://apod.nasa.gov/apod/image/9702/betelgeuse_hst.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +2017-05-19,"Named for the three astronomers instrumental in its discovery and identification, Wolf - Lundmark - Melotte (WLM) is a lonely dwarf galaxy. Seen toward the mostly southern constellation Cetus, about 3 million light-years from the Milky Way, it is one of the most remote members of our local galaxy group. In fact, it may never have interacted with any other local group galaxy. Still, telltale pinkish star forming regions and hot, young, bluish stars speckle the isolated island universe. Older, cool yellowish stars fade into the small galaxy's halo, extending about 8,000 light-years across. This sharp portrait of WLM was captured by the 268-megapixel OmegaCAM widefield imager and survey telescope at ESO's Paranal Observatory.",https://apod.nasa.gov/apod/image/1705/eso1610a_WLMgalaxy.jpg,image,v1,Wolf-Lundmark-Melotte,https://apod.nasa.gov/apod/image/1705/eso1610a_WLMgalaxy1024.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +2021-06-26,"These two panels, composed of video frames made with a safe solar telescope and hydrogen alpha filter, show remarkably sharp details on the solar disk and giant prominences along the Sun's edge on June 6 (top) and June 18. Taken from Beijing, China, they also show a transit of the International Space Station and China's new Tiangong Space Station in silhouette against the bright Sun. The International Space Station is near center in the bottom panel, crossing the solar disk left of bright active region AR2833 and below a large looping solar filament. China's space station is below solar active region AR2827 and right of center in the top panel, seen as a smaller, combined ""+"" and ""-"" shape. The pictures of the transiting orbital outposts were taken with the same equipment and at the same pixel scale, with the International Space Station some 492 kilometers away. China's space station was over 400 kilometers from the camera.",https://apod.nasa.gov/apod/image/2106/ISS_CSSsolarTransit.jpg,image,v1,Pixels in the Sun,https://apod.nasa.gov/apod/image/2106/ISS_CSSsolarTransit_1070.jpg,Wang Letian,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +2001-06-30,"Stars like the Sun use hydrogen for fuel, ""burning"" hydrogen into helium at their cores through nuclear fusion. But what happens when that hydrogen runs out? For a while, hydrogen burns in a shell surrounding the stellar core and the star expands to become a red giant. The bright reddish-orange stars in this beautiful two-color composite picture of the old globular star cluster M10 are examples of this phase of stellar evolution. Yet the bright blue stars apparent in M10 have evolved beyond the simple, hydrogen shell burning stage. These stars have become ""horizontal branch"" giants with core temperatures hot enough to burn helium into carbon. In this image, only the barely visible, faint, gray-looking stars are likely to still be burning hydrogen at their cores.",https://apod.nasa.gov/apod/image/0106/m10_crednerkohle_big.jpg,image,v1,"Hydrogen, Helium, and the Stars of M10",https://apod.nasa.gov/apod/image/0106/m10_crednerkohle.jpg," +Till Credner, Sven Kohle +(Bonn University), +Hoher List Observatory +",exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +2016-10-01,"After closely following comet 67P/Churyumov-Gerasimenko for 786 days as it rounded the Sun, the Rosetta spacecraft's controlled impact with the comet's surface was confirmed by the loss of signal from the spacecraft on September 30, 2016. One of the images taken during its final descent, this high resolution view looks across the comet's stark landscape. The scene spans just over 600 meters (2,000 feet), captured when Rosetta was about 16 kilometers from the comet's surface. Rosetta's descent to the comet brought to an end the operational phase of an inspirational mission of space exploration. Rosetta deployed a lander to the surface of one of the Solar System's most primordial worlds and witnessed first hand how a comet changes when subject to the increasing intensity of the Sun's radiation. The decision to end the mission on the surface is a result of the comet's orbit now taking it to the dim reaches beyond Jupiter where there would be a lack of power to operate the spacecraft. Mission operators also faced an approaching period where the Sun would be close to line-of-sight between Earth and Rosetta, making radio communications increasingly difficult.",https://apod.nasa.gov/apod/image/1610/Comet67p_from_16_km2048.jpg,image,v1,Rosetta's Farewell,https://apod.nasa.gov/apod/image/1610/Comet67p_from_16_km1024.jpg," +ESA, +Rosetta, +MPS, OSIRIS; +UPD/LAM/IAA/SSO/INTA/UPM/DASP/IDA + +",exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +2019-07-05,"The road to the high mountaintop La Silla Observatory in the Chilean Atacama Desert also led in to the path of July 2nd's total solar eclipse. Recorded at regular intervals before and after the total eclipse phase, the frames in this composite sequence include the moment the Moon's dark shadow fell across some of planet Earth's advanced large telescopes. The dreamlike view looks west toward the setting Sun and the approaching Moon shadow. In fact La Silla was a little north of the shadow track's center line, so the region's stunning, clear skies are slightly brighter to the north (right) in the scene.",https://apod.nasa.gov/apod/image/1907/2019_07_02_TSE_LaSilla_Sequence_1500px.jpg,image,v1,La Silla Eclipse Sequence,https://apod.nasa.gov/apod/image/1907/2019_07_02_TSE_LaSilla_Sequence_1024px.jpg,"Petr +Horálek",exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +2007-10-03,"Swinging inside the orbit of Mercury, on April 20th periodic comet Encke encountered a blast from the Sun in the form of a Coronal Mass Ejection (CME). When CMEs, enormous clouds of energetic particles ejected from the Sun, slam into Earth's magnetosphere, they often trigger auroral displays. But in this case, the collison carried the tail of the comet away. The tail was likely ripped off by interacting magnetic fields rather than the mechanical pressure of the collision. Clicking on the two panel image will play a movie gif of the remarkable event as recorded by the Heliospheric Imager onboard the STEREO A spacecraft. In the movie, the time between frames is about 45 minutes, while the frames span about 14x20 million kilometers at the distance of the comet. Of course, similar collisions have happened before as the ancient comet loops through its 3.3 year solar orbit. So don't worry, Encke's tail grows back!",https://apod.nasa.gov/apod/image/0710/enckeRipoff_movie_short.gif,image,v1,Comet Encke's Tail Ripped Off,https://apod.nasa.gov/apod/image/0710/enckeRipoff_panel.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +1996-11-14,"A massive star ends life as a supernova, blasting its outer layers back to interstellar space. The spectacular death explosion is initiated by the collapse of what has become an impossibly dense stellar core. However, this core is not necessarily destroyed. Instead, it may be transformed into an exotic object with the density of an atomic nucleus but more total mass than the sun - a neutron star. Directly viewing a neutron star is difficult because it is small (roughly 10 miles in diameter) and therefore dim, but newly formed in this violent crucible it is intensely hot, glowing in X-rays. Images from the ROSAT X-ray observatory above may offer a premier view of such a recently formed neutron stars' X-ray glow. Pictured is the supernova remnant Puppis A, one of the brightest sources in the X-ray sky, with shocked gas clouds still expanding and radiating X-rays. In the inset close-up view, a faint pinpoint source of X-rays is visible which is most likely the young neutron star, kicked out by the asymmetric explosion and moving away from the site of the original supernova at about 600 miles per second.",https://apod.nasa.gov/apod/image/9611/puppisa_rosat_big.gif,image,v1,Supernova Remnant and Neutron Star,https://apod.nasa.gov/apod/image/9611/puppisa_rosat.gif,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +2013-12-27,"Cosmic clouds seem to form fantastic shapes in the central regions of emission nebula IC 1805. Of course, the clouds are sculpted by stellar winds and radiation from massive hot stars in the nebula's newborn star cluster, Melotte 15. About 1.5 million years young, the cluster stars are near the center of this colorful skyscape, along with dark dust clouds in silhouette. Dominated by emission from atomic hydrogen, the telescopic view spans about 30 light-years. But wider field images reveal that IC 1805's simpler, overall outline suggests its popular name - The Heart Nebula. IC 1805 is located along the northern Milky Way, about 7,500 light years distant toward the constellation Cassiopeia.",https://apod.nasa.gov/apod/image/1312/LRGBV6Melotte15_JWalker.jpg,image,v1,Melotte 15 in the Heart,https://apod.nasa.gov/apod/image/1312/LRGBV6Melotte15_JWalker900.jpg,Jimmy Walker,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +2015-05-16,"This close-up from the Mars Reconnaissance Orbiter's HiRISE camera shows weathered craters and windblown deposits in southern Acidalia Planitia. A striking shade of blue in standard HiRISE image colors, to the human eye the area would probably look grey or a little reddish. But human eyes have not gazed across this terrain, unless you count the eyes of NASA astronauts in the scifi novel The Martian by Andy Weir. The novel chronicles the adventures of Mark Watney, an astronaut stranded at the fictional Mars mission Ares 3 landing site corresponding to the coordinates of this cropped HiRISE frame. For scale Watney's 6-meter-diameter habitat at the site would be about 1/10th the diameter of the large crater. Of course, the Ares 3 landing coordinates are only about 800 kilometers north of the (real life) Carl Sagan Memorial Station, the 1997 Pathfinder landing site.",https://apod.nasa.gov/apod/image/1505/PIA19363.jpg,image,v1,Ares 3 Landing Site: The Martian Revisited,https://apod.nasa.gov/apod/image/1505/PIA19363_1024.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +2022-11-21,"Stars can make beautiful patterns as they age -- sometimes similar to flowers or insects. NGC 6302, the Butterfly Nebula, is a notable example. Though its gaseous wingspan covers over 3 light-years and its estimated surface temperature exceeds 200,000 degrees C, the aging central star of NGC 6302, the featured planetary nebula, has become exceptionally hot, shining brightly in visible and ultraviolet light but hidden from direct view by a dense torus of dust. This sharp close-up was recorded by the Hubble Space Telescope and is processed here to show off remarkable details of the complex planetary nebula, highlighting in particular light emitted by oxygen (shown as blue), hydrogen (green), and nitrogen (red). NGC 6302 lies about 3,500 light-years away in the arachnologically correct constellation of the Scorpion (Scorpius). Planetary nebulas evolve from outer atmospheres of stars like our Sun, but usually fade in about 20,000 years.",https://apod.nasa.gov/apod/image/2211/Butterfly_HubbleOstling_3656.jpg,image,v1,The Butterfly Nebula from Hubble,https://apod.nasa.gov/apod/image/2211/Butterfly_HubbleOstling_960.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +1999-08-19,"Only in the fleeting darkness of a total solar eclipse is the light of the solar corona easily visible from Earth. Normally overwhelmed by the bright solar disk, the expansive corona, the sun's outer atmosphere, is an alluring sight. But the subtle details and extreme ranges in the corona's brightness discernible to the eye are notoriously difficult to photograph. In this series of images recorded from Siofok, Hungary during the total phase of the August 11 eclipse, progressively longer exposures (top left to bottom center) have been used to more faithfully capture different regions of the elusive solar corona. The final image (at bottom right) shows light from the solar disk emerging from behind the moon's edge at the end of totality.",https://apod.nasa.gov/apod/image/9908/augeclipse_cagas_big.jpg,image,v1,Light From The Dark Sun,https://apod.nasa.gov/apod/image/9908/augeclipse_cagas.jpg," +Pavel and Roman Cagas +",exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +1999-07-05,"As Mars rotates, most of its surface becomes visible. During Earth's recent pass between Mars and the Sun, the Hubble Space Telescope was able to capture the most detailed time-lapse pictures ever from the Earth. Dark and light sand and gravel create an unusual blotted appearance for the red planet. Winds cause sand-tinted features on the Martian surface to shift over time. Visible in the above pictures are the north polar cap, made of water ice and dry ice, clouds including an unusual cyclone, and huge volcanoes leftover from ancient times. The Mars Global Surveyor satellite orbiting Mars continues to scan the surface for good places to land future robot explorers.",https://apod.nasa.gov/apod/image/9907/mars4_hst_big.jpg,image,v1,Four Faces of Mars,https://apod.nasa.gov/apod/image/9907/mars4_hst.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +2013-06-29,"Once known as Earth's sunset comet, PanSTARRS (C/2011 L4) is up all night now, but only for northern hemisphere skygazers. Telescopes are required to track its progress as it fades and heads for the outer solar system. But because planet Earth passed through the comet's orbital plane in late May, PanSTARRS will also be remembered for its remarkably long anti-tail. That edge-on perspective looking along the broad, fanned-out dust tail as it trailed behind the comet created the appearance of an anti-tail pointing in the sunward direction, back toward the inner solar system. Recorded on the night of May 27, this 13 pane mosaic (shown in positive and negative views) follows PanSTARRS' anti-tail as it stretches over 7 degrees from the comet's coma at the far right. The anti-tail was likely much longer, but gets lost in the evening's bright moonlight encroaching on the left edge of the scene. Background star cluster NGC 188 in Cepheus shows up along the way, near top left.",https://apod.nasa.gov/apod/image/1306/C2011-L4-PANSTARRS_33pcntLawrence.jpg,image,v1,PanSTARRS: The Anti Tail Comet,https://apod.nasa.gov/apod/image/1306/C2011-L4-PANSTARRS_600Lawrence.jpg,Digital-Astronomy,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +1996-08-13,"Voyager spacecraft images of Europa's surface, like the one above, are suggestive of sea ice on Earth. The criss-crossing dark streaks may indeed be cracks in its ice-covered surface caused by Jupiter's tidal stresses accompanied by the freezing and expansion of an underlying layer of water. This tantalizing prospect of oceans of liquid water beneath its frozen surface has helped make the smallest of the Galilean moon's of Jupiter a planned focus of the Galileo spacecraft's ongoing mission to explore the Jovian system. New Europa images and results from the Galileo mission were released today revealing details which further suggest that Europa's icy surface was once - and may still be - supported on slush or liquid water.",https://apod.nasa.gov/apod/image/europa3_vg_big.jpg,image,v1,Europa's Surface,https://apod.nasa.gov/apod/image/europa3_vg.gif,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +2006-06-03,"The pixelated planet above is actually our own planet Earth seen in gamma rays - the most energetic form of light. In fact, the gamma rays used to construct this view pack over 35 million electron volts (MeV) compared to a mere two electron volts (eV) for a typical visible light photon. The Earth's gamma-ray glow is indeed very faint, and this image was constructed by combining data from seven years of exposure during the life of the Compton Gamma Ray Observatory, operating in Earth orbit from 1991 to 2000. Brightest near the edge and faint near the center, the picture indicates that the gamma rays are coming from high in Earth's atmosphere. The gamma rays are produced as the atmosphere interacts with high energy cosmic rays from space, blocking the harmful radiation from reaching the surface. Astronomers need to understand Earth's gamma-ray glow well as it can interfere with observations of cosmic gamma-ray sources like pulsars, supernova remnants, and distant active galaxies powered by supermassive black holes.",https://apod.nasa.gov/apod/image/0606/grayEarth_petry.jpg,image,v1,Gamma-Ray Earth,https://apod.nasa.gov/apod/image/0606/grayEarth_petry.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +2020-11-07,"These are galaxies of the Hercules Cluster, an archipelago of island universes a mere 500 million light-years away. Also known as Abell 2151, this cluster is loaded with gas and dust rich, star-forming spiral galaxies but has relatively few elliptical galaxies, which lack gas and dust and the associated newborn stars. The colors in this deep composite image clearly show the star forming galaxies with a blue tint and galaxies with older stellar populations with a yellowish cast. The sharp picture spans about 1/2 degree across the cluster center, corresponding to over 4 million light-years at the cluster's estimated distance. Diffraction spikes around brighter foreground stars in our own Milky Way galaxy are produced by the imaging telescope's mirror support vanes. In the cosmic vista many galaxies seem to be colliding or merging while others seem distorted - clear evidence that cluster galaxies commonly interact. In fact, the Hercules Cluster itself may be seen as the result of ongoing mergers of smaller galaxy clusters and is thought to be similar to young galaxy clusters in the much more distant, early Universe.",https://apod.nasa.gov/apod/image/2011/Abell2151_Howard_Trottier_2020_FFTelescope1024.jpg,image,v1,The Hercules Cluster of Galaxies,https://apod.nasa.gov/apod/image/2011/Abell2151_Howard_Trottier_2020_FFTelescope1024.jpg,Howard Trottier,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +2020-01-06,"Some cloud patterns on Jupiter are quite complex. The featured tumultuous clouds were captured in May by NASA's robotic Juno spacecraft currently orbiting our Solar System's largest planet. The image was taken when Juno was only about 15,000 kilometers over Jupiter's cloud tops, so close that less than half of the giant planet is visible. The rough white clouds on the far right are high altitude clouds known as pop-up clouds. Juno's mission, now extended into 2021, is to study Jupiter in new ways. Among many other things, Juno has been measuring Jupiter's gravitational field, finding surprising evidence that Jupiter may be mostly a liquid.",https://apod.nasa.gov/apod/image/2001/JupiterClouds_JunoGill_2295.jpg,image,v1,Tumultuous Clouds of Jupiter,https://apod.nasa.gov/apod/image/2001/JupiterClouds_JunoGill_960.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +1999-11-02,"A night sky can glow in fascinating ways. Through a clearing in the woods, the pictured sky above Alaska shines by reflected light from a nearby city, by the brightness of the Moon, and by aurora. The night sky in or near a city appears to contain relatively few stars because lights there reflect off atmospheric particles, hiding stars in a diffuse glow. The bright Moon also creates a diffuse sky glow, although much less bright than the analogous blue-sky glow created during the day by the Sun. Particles from the Sun crashing into the Earth's atmosphere are seen here as bands of aurora. These glows also illuminate visible clouds. Auroral displays are becoming more frequent as the Sun approaches Solar Maximum.",https://apod.nasa.gov/apod/image/9911/auroramoon_curtis.jpg,image,v1,Aurora Through a Moonlit Sky,https://apod.nasa.gov/apod/image/9911/auroramoon_curtis_big.jpg," +Jan Curtis +(U. Alaska), +ACRC +",exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +2013-06-15,"Over a five hour period last Tuesday morning, exposures captured this tantalizing view of meteor streaks and the Milky Way in dark skies above Las Campanas Observatory in Chile. During that time, astronomers had hoped to see an outburst from the gamma Delphinid meteor shower as Earth swept through the dust trail left by an unknown comet. Named for the shower's radiant point in the constellation Delphinus, a brief but strong outburst was reported in bright, moonlit skies on June 10, 1930. While no strong Delphinid meteor activity was reported since, an outburst was tentatively predicted to occur again in 2013. But even though Tuesday's skies were dark, the overall rate of meteors in this field is low, and only the three lower meteor streaks seem to point back to the shower's estimated radiant.",https://apod.nasa.gov/apod/image/1306/delphinids_lcBeletsky.jpg,image,v1,Delphinid Meteor Mystery,https://apod.nasa.gov/apod/image/1306/delphinids_lcBeletsky900.jpg,Yuri Beletsky,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +2019-05-09,"""Beautiful Nebula discovered between the Balance [Libra] & the Serpent [Serpens] ..."" begins the description of the 5th entry in 18th century astronomer Charles Messier's famous catalog of nebulae and star clusters. Though it appeared to Messier to be fuzzy and round and without stars, Messier 5 (M5) is now known to be a globular star cluster, 100,000 stars or more, bound by gravity and packed into a region around 165 light-years in diameter. It lies some 25,000 light-years away. Roaming the halo of our galaxy, globular star clusters are ancient members of the Milky Way. M5 is one of the oldest globulars, its stars estimated to be nearly 13 billion years old. The beautiful star cluster is a popular target for earthbound telescopes. Even close to its dense core, the cluster's red and blue giant stars, and rejuvenated blue stragglers stand out with yellowish and blue hues in this sharp color image.",https://apod.nasa.gov/apod/image/1905/m5sBlock.jpg,image,v1,Messier 5,https://apod.nasa.gov/apod/image/1905/m5sBlock1024.jpg,Adam Block,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +2004-11-19,"This moon is doomed. Mars, the red planet named for the Roman god of war, has two tiny moons, Phobos and Deimos, whose names are derived from the Greek for Fear and Panic. These martian moons may well be captured asteroids originating in the main asteroid belt between Mars and Jupiter or perhaps from even more distant reaches of the Solar System. The largest moon, Phobos, is indeed seen to be a cratered, asteroid-like object in this stunning new color image from the Mars Express spacecraft, recorded at a resolution of about seven meters per pixel. But Phobos orbits so close to Mars - about 5,800 kilometers above the surface compared to 400,000 kilometers for our Moon - that gravitational tidal forces are dragging it down. In 100 million years or so it will likely crash into the surface or be shattered by stress caused by the relentless tidal forces, the debris forming a ring around Mars.",https://apod.nasa.gov/apod/image/0411/Phobos_hiresME_full.jpg,image,v1,Phobos: Doomed Moon of Mars,https://apod.nasa.gov/apod/image/0411/Phobos_hiresME_c1.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +2020-09-05,"Illuminating planet Earth's night, full moons can have many names. This year the last full moon of northern hemisphere summer was on September 2, known to some as the Full Corn Moon. A few days earlier on August 30 this almost full moon rose just before sunset though, shining through cloudy skies over Cape Canaveral Air Force Station on Florida's Space Coast. A well-timed snapshot caught the glare of rocket engines firing below the lunar disk, a Falcon 9 rocket's first stage successfully returning to Cape Canaveral's landing zone 1. About 9 minutes earlier, the same SpaceX Falcon 9 rocket had launched the SAOCOM 1B satellite toward polar orbit. The fourth launch for this reusable Falcon 9 first stage, it was the first launch to a polar orbit from Cape Canaveral since 1969.",https://apod.nasa.gov/apod/image/2009/Falcon9MoonKatieDarby.jpg,image,v1,A Falcon 9 Moon,https://apod.nasa.gov/apod/image/2009/Falcon9MoonKatieDarby1200.jpg,Katie Darby,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +1998-06-25,"This strangely distorted galaxy of stars is cataloged as NGC 4650A. It lies about 165 million light-years away in the southern constellation Centaurus. The complex system seems to have at least two parts, a flattened disk of stars with a dense, bright, central core and a sparse, sharply tilted ring of gas, dust and stars. Observations show that the stars in the disk and the stars and gas in the ring really do move in two different, nearly perpendicular planes, probably as the result of a past galaxy vs. galaxy collision. The observed motions within both disk and ring also indicate the presence of ""dark matter"" - an unseen source of gravity which influences the movement of this system's visible stars. Over the decades evidence that our Universe is largely composed of such dark matter has grown while the nature of dark matter has remained a profound astrophysical mystery. The picture was constructed from images made using part of the European Southern Observatory's (ESO) new Very Large Telescope system now undergoing its testing phase.",https://apod.nasa.gov/apod/image/9806/ngc4650a_vlt_big.jpg,image,v1,NGC 4650A: Strange Galaxy and Dark Matter,https://apod.nasa.gov/apod/image/9806/ngc4650a_vlt.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +1996-12-27,"Most of our universe is too dim to see. To peer into our cosmos' unknown depths, astronomers must deploy new tools - and the classic new tool is a larger telescope. Pictured above is the new Hobby-Eberly Telescope (HET) which recently declared ""first light"" in western Texas. HET currently has the largest single mirror of any optical telescope -- 11 meters in diameter. Telescopes in space, like the Hubble Space Telescope, are much smaller but avoid the Earth's atmosphere blurring out fine detail. HET's huge size, on the other hand, allows it to see very dim objects and determine their spectrum. HET's unusual design allows the primary mirror to stay put during an observation! Only smaller focusing instruments suspending above the primary move to track an astronomical object. ",https://apod.nasa.gov/apod/image/9612/het_ut_big.jpg,image,v1,HET: The New Largest Optical Telescope,https://apod.nasa.gov/apod/image/9612/het_ut.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +1999-01-15,"The Orion Nebula and its surroundings present skygazers with a wondrous jumble of newborn stars, gas, and dust. Emission nebulae - glowing energized clouds of gas, and reflection nebulae - dust clouds shining by reflected starlight, abound at this photogenic cosmic location a mere 1,500 light-years or so away. This telescopic image reveals an intriguing nebulosity which seems to consist of dust clouds illuminated not by starlight but by the light of the Orion Nebula itself. In non-telescopic views, the bright group of stars near the top appear as the northernmost star in Orion's sword. They are seen here illuminating the nearby dust clouds. Yet the yellowish streamers of dust across the middle reflect the light of the Orion Nebula, which lies just off the bottom edge of the photo.",https://apod.nasa.gov/apod/image/9901/uks025b_malin.jpg,image,v1,Reflections Of Orion,https://apod.nasa.gov/apod/image/9901/uks025b_malin.jpg," + +David Malin (AAO), +AATB, +ROE, +UKS Telescope +",exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +2010-07-29,"From central Australia, this serene 360 degree panorama follows a clear horizon as twilight began on May 28. At left, a bright western sky is still illuminated by the setting Sun. But sweeping right, toward a view centered on the countryside's dominating sandstone formation called Uluru or Ayers Rock, the sky takes on progressively darker hues and subtle colors. Behind Uluru is the shadow of planet Earth itself, a dark blue arch rising in the east. Cast through the dense atmosphere and still close to the horizon, Earth's long shadow is bounded above by a pinkish glow or antitwilight arch. Known as the Belt of Venus, the lovely color of the antitwilight arch is due to backscattering of reddened light from the setting Sun. On that night, a nearly full Moon also rose above Earth's shadow in the eastern sky.",https://apod.nasa.gov/apod/image/1007/BeltOfVenusPan_ward.jpg,image,v1,"Sunset, Shadowrise",https://apod.nasa.gov/apod/image/1007/BeltOfVenusPan_ward600h.jpg,Barden Ridge Observatory,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +2013-03-18,"Have you seen the comet? As Comet PANSTARRS fades, careful observers -- even with unaided eyes -- should still be able to find the shedding ice ball on the western horizon just after sunset. Pictured above, Comet PANSTARRS (C/2011 L4) was pointed out from a hilltop last week on First Encounter Beach in Massachusetts, USA. The comet was discovered by -- and is named for -- the Pan-STARRS astronomical sky survey that discovered it. As the comet now recedes from both the Earth and the Sun, it will remain visible further into the night, although binoculars or a small telescope will soon to be needed to find it. Growing Gallery: Comet PanSTARRS at Sunset",https://apod.nasa.gov/apod/image/1303/panstarrs_cook_1100.jpg,image,v1,Comet PANSTARRS Just After Sunset,https://apod.nasa.gov/apod/image/1303/panstarrs_cook_960.jpg," +Chris Cook +",exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +2010-12-04,"In dwindling twilight at an August day's end, these broad dark bands appeared in the sky for a moment, seen from Robert Smithson's Spiral Jetty on the eastern shore of Utah's Great Salt Lake. Outlined by rays of sunlight known as crepuscular rays, they are actually shadows cast by clouds near the distant western horizon, the setting Sun having disappeared from direct view behind them. The cloud shadows are parallel, but seem to converge in the distance because of perspective. Coiled in the salt-encrusted lake surface, Smithson's most famous earthwork provides a dramatic contrast to the converging lines. The Spiral Jetty was constructed in 1970, when the water level was unusually low and was completely submerged in a few years as the level rose. Now just above water again, it has spent much of its existence submerged in the briny lake.",https://apod.nasa.gov/apod/image/1012/SpiralRays_erisoty.jpg,image,v1,Sunset at the Spiral Jetty,https://apod.nasa.gov/apod/image/1012/SpiralRays_erisoty.jpg,Arne Erisoty,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +2018-03-02,"Colourful star trails arc through the night in this wide-angle mountain and skyscape. From a rotating planet, the digitally added consecutive exposures were made with a camera fixed to a tripod and looking south, over northern Iran's Alborz Mountain range. The stars trace concentric arcs around the planet's south celestial pole, below the scene's rugged horizon. Combined, the many short exposures also bring out the pretty star colours. Bluish trails are from stars hotter than our Sun, while yellowish trails are from cooler stars. Near the center, the remarkably pinkish trail was traced by the star-forming Orion Nebula.",https://apod.nasa.gov/apod/image/1803/SGU-Colourful_Alboraz_Startrails-1600-cp70.jpg,image,v1,Alborz Mountain Star Trails,https://apod.nasa.gov/apod/image/1803/SGU-Colourful_Alboraz_Startrails-900-cp60.jpg,Stéphane Guisard,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +2022-08-29,"The famous Horsehead Nebula in Orion is not alone. A deep exposure shows that the dark familiar shaped indentation, visible just right of center, is part of a vast complex of absorbing dust and glowing gas. The featured spectacular picture details an intricate tapestry of gaseous wisps and dust-laden filaments that were created and sculpted over eons by stellar winds and ancient supernovas. The Flame Nebula is visible in orange just to the Horsehead's left. To highlight the dust and gas, most of the stars have been digitally removed, although a notable exception is Alnitak, just above the Flame Nebula, which is the rightmost star in Orion's famous belt of three aligned stars. The Horsehead Nebula lies 1,500 light years distant towards the constellation of Orion. NASA Coverage: Artemis I Mission to the Moon Teachers & Students: Ideas for utilizing APOD in the classroom",https://apod.nasa.gov/apod/image/2208/Horsehead_Chatzifrantzis_2500.jpg,image,v1,The Horsehead Nebula Region without Stars,https://apod.nasa.gov/apod/image/2208/Horsehead_Chatzifrantzis_1080.jpg," +George Chatzifrantzis +",exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +2012-08-13,"What would it be like to fly through the universe? Possibly the best simulated video of this yet has been composed from recently-released galaxy data from the Sloan Digital Sky Survey. Every spot in the above video is a galaxy containing billions of stars. Many galaxies are part of huge clusters, long filaments, or small groups, while expansive voids nearly absent of galaxies also exist. The movie starts by flying right through a large nearby cluster of galaxies and later circles the SDSS-captured universe at about 2 billion light years (a redshift of about 0.15) from Earth. Analyses of galaxy positions and movements continues to bolster the case that our universe contains not only the bright matter seen, like galaxies, but also a significant amount of unseen dark matter and dark energy.",,video,v1,A Flight Through the Universe,https://www.youtube.com/embed/08LBltePDZw?rel=0,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +2021-04-02,"Gorgeous spiral galaxy NGC 3521 is a mere 35 million light-years away, toward the constellation Leo. Relatively bright in planet Earth's sky, NGC 3521 is easily visible in small telescopes but often overlooked by amateur imagers in favor of other Leo spiral galaxies, like M66 and M65. It's hard to overlook in this colorful cosmic portrait, though. Spanning some 50,000 light-years the galaxy sports characteristic patchy, irregular spiral arms laced with dust, pink star forming regions, and clusters of young, blue stars. Remarkably, this deep image also finds NGC 3521 embedded in gigantic bubble-like shells. The shells are likely tidal debris, streams of stars torn from satellite galaxies that have undergone mergers with NGC 3521 in the distant past.",https://apod.nasa.gov/apod/image/2104/NGC3521-LRGB-1.jpg,image,v1,NGC 3521: Galaxy in a Bubble,https://apod.nasa.gov/apod/image/2104/NGC3521-LRGB-1024c.jpg,Eric Benson,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +2010-12-26,"Orion always comes up sideways ... and was caught in the act earlier this month by over a snowy landscape in Donegal, Ireland. To compose this serene picture, the photographer found a picturesque setting to the east, waited until after sunset, and then momentarily lit the foreground with a flashlight. The three bright stars in Orion's belt stand in a nearly vertical line above the snow covered road at the bottom. Hanging from his belt, the stars and nebulae of the Hunter's sword are visible lower and to the right. Yellow-orange Betelgeuse is the brightest star on the image left. As winter progresses in Earth's northern hemisphere, Orion will rise earlier and so appear continually higher in the sky at sunset. Best Astronomy Images: APOD Editor to speak in Philadelphia on Jan 5 and New York City on Jan 7",https://apod.nasa.gov/apod/image/1012/snowyorion_alexander_big.jpg,image,v1,Sideways Orion Over Snowy Ireland,https://apod.nasa.gov/apod/image/1012/snowyorion_alexander.jpg," +Brendan Alexander +(Donegal Skies) +",exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +2000-07-26,"As the Moon passed almost directly through the center of Earth's shadow on July 16th, sky gazers in the Pacific hemisphere were graced by a lingering lunar eclipse. The total phase lasted 1 hour and 47 minutes, the longest since 1859. A longer total lunar eclipse won't occur until the year 3000. Taking advantage of the lengthy totality, astronomer and photographer, Noel Munford used a small telescope to record this colourful picture of the eclipsed Moon and nearby stars in the skies above Palmerston North, New Zealand. Near the top in this southern hemisphere perspective is the 84 kilometer wide bright ray crater Tycho. The Moon looks red even when it lies completely in shadow because it is still illuminated by sunlight reddened by dust and refracted by the atmosphere along the Earth's limb. Changes in atmospheric dust content mean that each eclipse can have a different appearance. An experienced observer, Munford comments that at mid totality this eclipse had a more uniform, delicate, subtle colour and was one of the lightest he has seen.",https://apod.nasa.gov/apod/image/0007/nzeclipse_munford_big.jpg,image,v1,Lingering Lunar Eclipse,https://apod.nasa.gov/apod/image/0007/nzeclipse_munford.jpg," +Noel Munford +(Palmerston North Astronomical Society, New Zealand) + +",exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:38:30.986179 +,,,,,,,,star,{'self': 'http://api.nasa.gov/neo/rest/v1/neo/2000433?api_key=PBI6QS2eOkQigQpGPHNNCTxvPbSzakdW2Nq8R7yS'},2000433,2000433,433 Eros (A898 PA),Eros,433,https://ssd.jpl.nasa.gov/tools/sbdb_lookup.html#/?sstr=2000433,10.41,"{'kilometers': {'estimated_diameter_min': 22.0067027115, 'estimated_diameter_max': 49.2084832235}, 'meters': {'estimated_diameter_min': 22006.7027114738, 'estimated_diameter_max': 49208.4832234845}, 'miles': {'estimated_diameter_min': 13.6743268705, 'estimated_diameter_max': 30.5767244291}, 'feet': {'estimated_diameter_min': 72200.4705239119, 'estimated_diameter_max': 161445.1600989368}}",False,"[{'close_approach_date': '1900-12-27', 'close_approach_date_full': '1900-Dec-27 01:30', 'epoch_date_close_approach': -2177879400000, 'relative_velocity': {'kilometers_per_second': '5.5786191875', 'kilometers_per_hour': '20083.0290749201', 'miles_per_hour': '12478.8132604691'}, 'miss_distance': {'astronomical': '0.3149291693', 'lunar': '122.5074468577', 'kilometers': '47112732.928149391', 'miles': '29274494.7651919558'}, 'orbiting_body': 'Earth'}, {'close_approach_date': '1907-11-05', 'close_approach_date_full': '1907-Nov-05 03:31', 'epoch_date_close_approach': -1961526540000, 'relative_velocity': {'kilometers_per_second': '4.3944908885', 'kilometers_per_hour': '15820.1671985367', 'miles_per_hour': '9830.0366684463'}, 'miss_distance': {'astronomical': '0.4714855425', 'lunar': '183.4078760325', 'kilometers': '70533232.893794475', 'miles': '43827318.620434755'}, 'orbiting_body': 'Earth'}, {'close_approach_date': '1917-04-20', 'close_approach_date_full': '1917-Apr-20 21:19', 'epoch_date_close_approach': -1663036860000, 'relative_velocity': {'kilometers_per_second': '4.8167840184', 'kilometers_per_hour': '17340.4224662258', 'miles_per_hour': '10774.6641707501'}, 'miss_distance': {'astronomical': '0.499257206', 'lunar': '194.211053134', 'kilometers': '74687814.59975122', 'miles': '46408855.985038036'}, 'orbiting_body': 'Earth'}, {'close_approach_date': '1924-03-05', 'close_approach_date_full': '1924-Mar-05 22:13', 'epoch_date_close_approach': -1446083220000, 'relative_velocity': {'kilometers_per_second': '4.5960548855', 'kilometers_per_hour': '16545.797587763', 'miles_per_hour': '10280.915173352'}, 'miss_distance': {'astronomical': '0.3597864889', 'lunar': '139.9569441821', 'kilometers': '53823292.394218643', 'miles': '33444243.0636095534'}, 'orbiting_body': 'Earth'}, {'close_approach_date': '1931-01-30', 'close_approach_date_full': '1931-Jan-30 04:07', 'epoch_date_close_approach': -1228247580000, 'relative_velocity': {'kilometers_per_second': '5.9208185341', 'kilometers_per_hour': '21314.9467227704', 'miles_per_hour': '13244.2789789347'}, 'miss_distance': {'astronomical': '0.1740731458', 'lunar': '67.7144537162', 'kilometers': '26040971.835879446', 'miles': '16181109.5707945148'}, 'orbiting_body': 'Earth'}, {'close_approach_date': '1938-01-13', 'close_approach_date_full': '1938-Jan-13 22:04', 'epoch_date_close_approach': -1008726960000, 'relative_velocity': {'kilometers_per_second': '6.0840524046', 'kilometers_per_hour': '21902.5886564605', 'miles_per_hour': '13609.4168237879'}, 'miss_distance': {'astronomical': '0.2150052405', 'lunar': '83.6370385545', 'kilometers': '32164326.017637735', 'miles': '19985985.424901343'}, 'orbiting_body': 'Earth'}, {'close_approach_date': '1944-11-27', 'close_approach_date_full': '1944-Nov-27 01:41', 'epoch_date_close_approach': -791936340000, 'relative_velocity': {'kilometers_per_second': '3.626098636', 'kilometers_per_hour': '13053.9550896485', 'miles_per_hour': '8111.2200388986'}, 'miss_distance': {'astronomical': '0.4030090561', 'lunar': '156.7705228229', 'kilometers': '60289296.383270507', 'miles': '37462031.6350747166'}, 'orbiting_body': 'Earth'}, {'close_approach_date': '1961-04-04', 'close_approach_date_full': '1961-Apr-04 09:08', 'epoch_date_close_approach': -275928720000, 'relative_velocity': {'kilometers_per_second': '3.7078364482', 'kilometers_per_hour': '13348.2112136055', 'miles_per_hour': '8294.0593510317'}, 'miss_distance': {'astronomical': '0.4424921301', 'lunar': '172.1294386089', 'kilometers': '66195880.154722887', 'miles': '41132212.6021023606'}, 'orbiting_body': 'Earth'}, {'close_approach_date': '1968-02-11', 'close_approach_date_full': '1968-Feb-11 13:46', 'epoch_date_close_approach': -59566440000, 'relative_velocity': {'kilometers_per_second': '6.0668849725', 'kilometers_per_hour': '21840.7859008821', 'miles_per_hour': '13571.014994912'}, 'miss_distance': {'astronomical': '0.2662714057', 'lunar': '103.5795768173', 'kilometers': '39833635.134625859', 'miles': '24751473.1315964942'}, 'orbiting_body': 'Earth'}, {'close_approach_date': '1975-01-23', 'close_approach_date_full': '1975-Jan-23 07:39', 'epoch_date_close_approach': 159694740000, 'relative_velocity': {'kilometers_per_second': '5.8253076833', 'kilometers_per_hour': '20971.1076598791', 'miles_per_hour': '13030.6307567732'}, 'miss_distance': {'astronomical': '0.1511341909', 'lunar': '58.7912002601', 'kilometers': '22609353.042813383', 'miles': '14048800.5292673654'}, 'orbiting_body': 'Earth'}, {'close_approach_date': '1981-12-29', 'close_approach_date_full': '1981-Dec-29 08:05', 'epoch_date_close_approach': 378461100000, 'relative_velocity': {'kilometers_per_second': '5.6652718459', 'kilometers_per_hour': '20394.9786453535', 'miles_per_hour': '12672.6465921642'}, 'miss_distance': {'astronomical': '0.3084893271', 'lunar': '120.0023482419', 'kilometers': 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