diff --git "a/nasascraper_data.csv" "b/nasascraper_data.csv" --- "a/nasascraper_data.csv" +++ "b/nasascraper_data.csv" @@ -1,201 +1,190 @@ 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 -2017-04-10,"Why would this cluster of galaxy punch a hole in the cosmic microwave background (CMB)? First, the famous CMB was created by cooling gas in the early universe and flies right through most gas and dust in the universe. It is all around us. Large clusters of galaxies have enough gravity to contain very hot gas -- gas hot enough to up-scatter microwave photons into light of significantly higher energy, thereby creating a hole in CMB maps. This Sunyaev�Zel'dovich (SZ) effect has been used for decades to reveal new information about hot gas in clusters and even to help discover galaxy clusters in a simple yet uniform way. Pictured is the most detailed image yet obtained of the SZ effect, now using both ALMA to measure the CMB and the Hubble Space Telescope to measure the galaxies in the massive galaxy cluster RX J1347.5-1145. False-color blue depicts light from the CMB, while almost every yellow object is a galaxy. The shape of the SZ hole indicates not only that hot gas is present in this galaxy cluster, but also that it is distributed in a surprisingly uneven manner.",https://apod.nasa.gov/apod/image/1704/GalaxyClusterSZ_AlmaHubble_800.jpg,image,v1,Galaxy Cluster Gas Creates Hole in Microwave Background,https://apod.nasa.gov/apod/image/1704/GalaxyClusterSZ_AlmaHubble_960.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2024-04-02,"Only in the fleeting darkness of a total solar eclipse is the light of the solar corona easily visible. 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, although discernible to the eye, are notoriously difficult to photograph. Pictured here, however, using multiple images and digital processing, is a detailed image of the Sun's corona taken during the April 20, 2023 total solar eclipse from Exmouth, Australia. Clearly visible are intricate layers and glowing caustics of an ever changing mixture of hot gas and magnetic fields. Bright looping prominences appear pink just around the Sun's limb. A similar solar corona might be visible through clear skies in a narrow swath across the North America during the total solar eclipse that occurs just six days from today NASA Coverage: Total Solar Eclipse of 2024 April 8",https://apod.nasa.gov/apod/image/2404/CoronaExmouth_Hart_1920.jpg,image,v1,Detailed View of a Solar Eclipse Corona,https://apod.nasa.gov/apod/image/2404/CoronaExmouth_Hart_1080.jpg," -Phil Hart -",exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2017-10-29,"What spooky planet is this? Planet Earth of course, on a dark and stormy night in 2013 at Hverir, a geothermally active area along the volcanic landscape in northeastern Iceland. Geomagnetic storms produced the auroral display in the starry night sky while ghostly towers of steam and gas venting from fumaroles danced against the eerie greenish light. Tonight, there is also a chance for geomagnetic storms triggered by recent solar activity, so high-latitude skygazers should beware. Ghostly shapes may dance in your neighborhood pretty soon, too.",https://apod.nasa.gov/apod/image/1710/Hverir_Vetter_1300.jpg,image,v1,Night on a Spooky Planet,https://apod.nasa.gov/apod/image/1710/Hverir_Vetter_960.jpg,"Stéphane -Vetter",exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -1995-08-28,"August 28, 1995 Dusty Galaxy Centaurus A Credit: NOAO, Cerro Tololo Interamerican Observatory Explanation: One of the most unusual galaxies known, Centaurus A, is pictured above. Cen A is marked by dramatic dust lanes that run across the galaxy's center. These dust lanes are so thick they almost completely obscure the galaxy's center in visible light. Our Milky Way Galaxy contains dust, but not in the same proportion. Cen A is also unusual compared to a normal galaxy because it contains a higher proportion of young blue stars, is a very strong source of radio emission, and has a unique structure. Cen A is thought to be the result of the collision of two normal galaxies.",https://apod.nasa.gov/apod/image/cenA_ctio.gif,image,v1,Dusty Galaxy Centaurus A,https://apod.nasa.gov/apod/image/cenA_ctio.gif,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2012-01-20,"A Full Moon rising can be a dramatic celestial sight, and Full Moons can have many names. Captured on January 8 from Östersund, Sweden, this evocative moonrise portrait might make you feel the cold of winter in the north. If you can also imagine wolves howling in the distance then you probably understand why Native Americans would have called it the Wolf Moon, their traditional name for the first Full Moon in January. The photographer reports that no wolves were heard though, as he watched this beautiful Full Moon rise in fading light over the eastern horizon, echoing the yellow color of the setting Sun. Of course, due this year on February 7, the next Full Moon will be the Snow Moon.",https://apod.nasa.gov/apod/image/1201/GS_20120108_Moon_0010.jpg,image,v1,The Wolf's Moon,https://apod.nasa.gov/apod/image/1201/GS_20120108_Moon_0010_900.jpg,Göran Strand,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2000-05-25,"Since April 30, the robotic NEAR-Shoemaker spacecraft has been orbiting only 31 miles from asteroid Eros. Cruising over the asteroid's north and south poles at a leisurely 7 miles per hour, the spacecraft completes an orbit once every 1.2 earth days. This dramatic horizon view recorded by the spacecraft's camera on May 18 spans about 0.8 miles and reveals features as small as 13 feet across. Emphasized by long, harsh shadows produced by the low sun angle, the rolling surface of Eros is seen to be strewn with boulders and craters with a range of sizes. The jagged-looking boulder near the picture center is over 190 feet tall. While gathering sharp pictures of Eros' surface, experimenters will also take advantage of the close orbit to explore the asteroid's surface composition and internal structure, and search for a magnetic field.",https://apod.nasa.gov/apod/image/0005/near_00522.jpg,image,v1,Eros Horizon View,https://apod.nasa.gov/apod/image/0005/near_00522_sharp.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2020-06-11,"Big, beautiful, barred spiral galaxy NGC 1300 lies some 70 million light-years away on the banks of the constellation Eridanus. This Hubble Space Telescope composite view of the gorgeous island universe is one of the largest Hubble images ever made of a complete galaxy. NGC 1300 spans over 100,000 light-years and the Hubble image reveals striking details of the galaxy's dominant central bar and majestic spiral arms. In fact, on close inspection the nucleus of this classic barred spiral itself shows a remarkable region of spiral structure about 3,000 light-years across. Like other spiral galaxies, including our own Milky Way, NGC 1300 is thought to have a supermassive central black hole.",https://apod.nasa.gov/apod/image/2006/NGC1300HSTfull.jpg,image,v1,Barred Spiral Galaxy NGC 1300,https://apod.nasa.gov/apod/image/2006/NGC1300HST1200.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2008-11-27,"Large galaxies grow by eating small ones. Even our own galaxy practices galactic cannibalism, absorbing small galaxies that get too close and are captured by the Milky Way's gravity. In fact, the practice is common in the universe and well illustrated by this striking pair of interacting galaxies from the banks of the southern constellation Eridanus (The River). Located over 50 million light years away, the large, distorted spiral NGC 1532 is seen locked in a gravitational struggle with dwarf galaxy NGC 1531, a struggle the smaller galaxy will eventually lose. Seen edge-on, spiral NGC 1532 spans about 100,000 light-years. The NGC 1532/1531 pair is thought to be similar to the system of face-on spiral and small companion known as M51, the Whirlpool Galaxy.",https://apod.nasa.gov/apod/image/0811/NGC1532_gendler.jpg,image,v1,Galaxies in the River,https://apod.nasa.gov/apod/image/0811/NGC1532_gendler_c800.jpg,Robert Gendler,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2009-11-11,"Where can a telescope take you? Four hundred years ago, a telescope took Galileo to the Moon to discover craters, to Saturn to discover rings, to Jupiter to discover moons, to Venus to discover phases, and to the Sun to discover spots. Today, in celebration of Galileo's telescopic achievements and as part of the International Year of Astronomy, NASA has used its entire fleet of Great Observatories, and the Internet, to bring the center of our Galaxy to you. Pictured above, in greater detail and in more colors than ever seen before, are the combined images of the Hubble Space Telescope in near-infrared light, the Spitzer Space Telescope in infrared light, and the Chandra X-ray Observatory in X-ray light. A menagerie of vast star fields is visible, along with dense star clusters, long filaments of gas and dust, expanding supernova remnants, and the energetic surroundings of what likely is our Galaxy's central black hole. Many of these features are labeled on a complementary annotated image. Of course, a telescope's magnification and light-gathering ability create only an image of what a human could see if visiting these places. To actually go requires rockets.",https://apod.nasa.gov/apod/image/0911/galacticcenter_greatobs_big.jpg,image,v1,Great Observatories Explore Galactic Center,https://apod.nasa.gov/apod/image/0911/galacticcenter_greatobs.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2000-09-27,"Pictured above on September 3rd, the enclosure for the 8.2 meter telescope christened Yepun glints dramatically in the light of the setting sun. Later that evening, under dark skies at Paranal Observatory, Chile, astronomers and engineers successfully captured Yepun's first light images, making Yepun the fourth and final unit of the European Southern Observatory's Very Large Telescope (VLT) array to reach this milestone. Ultimately, the light from the three other 8.2 meter unit telescopes (Antu, Kueyen, and Melipal) will be combined with Yepun's to achieve an effective aperture of 16.4 meters -- creating the world's largest optical telescope. But the next major step will be to combine beams from two of the telescopes creating an interferometer. The upper part of the mostly subterranean interferometer lab is the building in front of the telescope enclosure. The VLT unit telescope names have been taken from the Mapuche language. Originally thought to refer to the bright star Sirius, the word Yepun is now believed by linguists to mean Venus or evening star.",https://apod.nasa.gov/apod/image/0009/yepun_esovlt_big.jpg,image,v1,Yepun,https://apod.nasa.gov/apod/image/0009/yepun_esovlt.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2023-07-20,"This magnificent spiral galaxy is Messier 64, often called the Black Eye Galaxy or the Sleeping Beauty Galaxy for its dark-lidded appearance in telescopic views. The spiral's central region, about 7,400 light-years across, is pictured in this reprocessed image from the Hubble Space Telescope. M64 lies some 17 million light-years distant in the otherwise well-groomed northern constellation Coma Berenices. The enormous dust clouds partially obscuring M64's central region are laced with young, blue star clusters and the reddish glow of hydrogen associated with star forming regions. But imposing clouds of dust 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 are likely the result of a billion year old merger of two different galaxies.",https://apod.nasa.gov/apod/image/2307/M64Hubble.jpg,image,v1,M64: The Black Eye Galaxy Close Up,https://apod.nasa.gov/apod/image/2307/M64Hubble1024.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2002-09-22,"Two hours before closest approach to Neptune in 1989, the Voyager 2 robot spacecraft snapped this picture. Clearly visible for the first time were long light-colored cirrus-type clouds floating high in Neptune's atmosphere. Shadows of these clouds can even be seen on lower cloud decks. Most of Neptune's atmosphere is made of hydrogen and helium, which is invisible. Neptune's blue color therefore comes from smaller amounts of atmospheric methane, which preferentially absorbs red light. Neptune has the fastest winds in the Solar System, with gusts reaching 2000 kilometers per hour. Speculation holds that diamonds may be created in the dense hot conditions that exist under the clouds-tops of Uranus and Neptune.",https://apod.nasa.gov/apod/image/0209/neptuneclouds_vg2_big.jpg,image,v1,Two Hours Before Neptune,https://apod.nasa.gov/apod/image/0209/neptuneclouds_vg2.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2012-04-12,"On another April 12th, in 1961, Soviet cosmonaut Yuri Alexseyevich Gagarin became the first human to see planet Earth from space. Commenting on his view from orbit he reported, ""The sky is very dark; the Earth is bluish. Everything is seen very clearly"". To celebrate, consider this recent image from the orbiting International Space Station. A stunning view of the planet at night from an altitude of 240 miles, it was recorded on March 28. The lights of Moscow, Russia are near picture center and one of the station's solar panel arrays is on the left. Aurora and the glare of sunlight lie along the planet's gently curving horizon. Stars above the horizon include the compact Pleiades star cluster, immersed in the auroral glow.",https://apod.nasa.gov/apod/image/1204/iss030e185321.jpg,image,v1,Yuri's Planet,https://apod.nasa.gov/apod/image/1204/iss030e185321_900.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2019-01-05,"On January 3, the Chinese Chang'e-4 spacecraft made the first successful landing on the Moon's farside. Taken by a camera on board the lander, this image is from the landing site inside Von Karman crater. It shows the desk-sized, six-wheeled Yutu 2 (Jade Rabbit 2) rover as it rolled down lander ramps and across the surface near local sunrise and the start of the two week long lunar day. Ripe for exploration, Von Karman crater itself is 186 kilometers in diameter. It lies within the Moon's old and deep South Pole-Aitken impact basin with some of the most ancient and least understood lunar terrains. To bridge communications from the normally hidden hemisphere of the Moon, China launched a relay satellite, Queqiao, in May of 2018 in to an orbit beyond the lunar farside.",https://apod.nasa.gov/apod/image/1901/Jan3yutu2CNSA.jpg,image,v1,Yutu 2 on the Farside,https://apod.nasa.gov/apod/image/1901/Jan3yutu2CNSA1024.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2007-09-03,"The many spectacular colors of the Rho Ophiuchi (oh'-fee-yu-kee) clouds highlight the many processes that occur there. The blue regions shine primarily by reflected light. Blue light from the star Rho Ophiuchi and nearby stars reflects more efficiently off this portion of the nebula than red light. The Earth's daytime sky appears blue for the same reason. The red and yellow regions shine primarily because of emission from the nebula's atomic and molecular gas. Light from nearby blue stars - more energetic than the bright star Antares - knocks electrons away from the gas, which then shines when the electrons recombine with the gas. The dark regions are caused by dust grains - born in young stellar atmospheres - which effectively block light emitted behind them. The Rho Ophiuchi star clouds, well in front of the globular cluster M4 visible above on far lower left, are even more colorful than humans can see - the clouds emits light in every wavelength band from the radio to the gamma-ray.",https://apod.nasa.gov/apod/image/0709/rhooph_noao_big.jpg,image,v1,The Colorful Clouds of Rho Ophiuchi,https://apod.nasa.gov/apod/image/0709/rhooph_noao.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2005-08-18,"Discovered in 1866, main belt asteroid 87 Sylvia lies 3.5 AU from the Sun, between the orbits of Mars and Jupiter. Also shown in recent years to be one in a growing list of double asteroids, new observations during August and October 2004 made at the Paranal Observatory convincingly demonstrate that 87 Sylvia in fact has two moonlets - the first known triple asteroid system. At the center of this composite of the image data, potato-shaped 87 Sylvia itself is about 380 kilometers wide. The data show inner moon, Remus, orbiting Sylvia at a distance of about 710 kilometers once every 33 hours, while outer moon Romulus orbits at 1360 kilometers in 87.6 hours. Tiny Remus and Romulus are 7 and 18 kilometers across respectively. Because 87 Sylvia was named after Rhea Silvia, the mythical mother of the founders of Rome, the discoverers proposed Romulus and Remus as fitting names for the two moonlets. The triple system is thought to be the not uncommon result of collisions producing low density, rubble pile asteroids that are loose aggregations of debris.",https://apod.nasa.gov/apod/image/0508/sylvia_compo680.jpg,image,v1,"Sylvia, Romulus and Remus",https://apod.nasa.gov/apod/image/0508/sylvia_compo680.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2022-04-12,"Massive stars, abrasive winds, mountains of dust, and energetic light sculpt one of the largest and most picturesque regions of star formation in the Local Group of Galaxies. Known as N11, the region is visible on the upper right of many images of its home galaxy, the Milky Way neighbor known as the Large Magellanic Cloud (LMC). The featured image was taken for scientific purposes by the Hubble Space Telescope and reprocessed for artistry. Although the section imaged above is known as NGC 1763, the entire N11 emission nebula is second in LMC size only to the Tarantula Nebula. Compact globules of dark dust housing emerging young stars are also visible around the image. A recent study of variable stars in the LMC with Hubble has helped to recalibrate the distance scale of the observable universe, but resulted in a slightly different scale than found using the pervasive cosmic microwave background. Astrophysicists: Browse 2,700+ codes in the Astrophysics Source Code Library",https://apod.nasa.gov/apod/image/2204/N11_HubbleLake_1600.jpg,image,v1,N11: Star Clouds of the LMC,https://apod.nasa.gov/apod/image/2204/N11_HubbleLake_960.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2004-06-27,"Two billion light-years away, galaxy cluster Abell 1689 is one of the most massive objects in the Universe. In this view from the Hubble Space Telescope's Advanced Camera for Surveys, Abell 1689 is seen to warp space as predicted by Einstein's theory of gravity -- bending light from individual galaxies which lie behind the cluster to produce multiple, curved images. The power of this enormous gravitational lens depends on its mass, but the visible matter, in the form of the cluster's yellowish galaxies, only accounts for about one percent of the mass needed to make the observed bluish arcing images of background galaxies. In fact, most of the gravitational mass required to warp space enough to explain this cosmic scale lensing is in the form of still mysterious dark matter. As the dominant source of the cluster's gravity, the dark matter's unseen presence is mapped out by the lensed arcs and distorted background galaxy images.",https://apod.nasa.gov/apod/image/0301/abell1689_hstacs_full.jpg,image,v1,Galaxy Cluster Abell 1689 Warps Space,https://apod.nasa.gov/apod/image/0301/abell1689_hstacs_c1.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2012-10-30,"Is this what will become of our Sun? Quite possibly. The bubble of expanding gas pictured above is the planetary nebula PK 164 +31.1, the remnants of the atmosphere of a Sun-like star expelled as its supply of fusion-able core hydrogen became depleted. Visible near the center of the nebula is what remains of the core itself -- a blue-hot white dwarf star. This particularly photogenic planetary nebula shows intricate shells of gas likely expelled at different times toward the end the star's demise, and whose structure is not fully understood. This deep image of PK 164 +31.1 from the Calar Alto Observatory in Spain shows many other stars from our own Milky Way Galaxy as well as several galaxies far in the distance. PK 164 +31, also known as Jones-Emberson 1, lies about 1,600 light years away toward the constellation of the Wildcat (Lynx). Due to its faintness (magnitude 17) and low surface brightness, the object is only visible with a good-sized telescope. Although the expanding nebula will fade away over the next few thousand years, the central white dwarf may well survive for billions of years -- to when our universe may be a very different place.",https://apod.nasa.gov/apod/image/1210/pk164_caha_1866.jpg,image,v1,Planetary Nebula PK 164 +31.1,https://apod.nasa.gov/apod/image/1210/pk164_caha_960.jpg," -Descubre Foundation, -CAHA, -OAUV, -DSA, -Vicent Peris (OAUV), -Jack Harvey (SSRO), -PixInsight -",exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2023-07-09,"Carinae may be about to explode. But no one knows when - it may be next year, it may be one million years from now. Eta Carinae's mass - about 100 times greater than our Sun - makes it an excellent candidate for a full blown supernova. Historical records do show that about 170 years ago Eta Carinae underwent an unusual outburst that made it one of the brightest stars in the southern sky. Eta Carinae, in the Keyhole Nebula, is the only star currently thought to emit natural LASER light. This featured image brings out details in the unusual nebula that surrounds this rogue star. Diffraction spikes, caused by the telescope, are visible as bright multi-colored streaks emanating from Eta Carinae's center. Two distinct lobes of the Homunculus Nebula encompass the hot central region, while some strange radial streaks are visible in red extending toward the image right. The lobes are filled with lanes of gas and dust which absorb the blue and ultraviolet light emitted near the center. The streaks, however, remain unexplained.",https://apod.nasa.gov/apod/image/2307/EtaCarinae_HubbleSchmidt_1764.jpg,image,v1,Doomed Star Eta Carinae,https://apod.nasa.gov/apod/image/2307/EtaCarinae_HubbleSchmidt_960.jpg," -NASA, -ESA, -Hubble; - Processing & -License: -Judy Schmidt -",exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2017-02-05,"Some moons wouldn't survive the collision. Tethys, one of Saturn's larger moons at about 1000 kilometers in diameter, survived the collision, but today exhibits the resulting expansive impact crater Odysseus. Sometimes called the Great Basin, Odysseus occurs on the leading hemisphere of Tethys and shows its great age by the relative amount of smaller craters that occur inside its towering walls. The density of Tethys is similar to water-ice. The featured image was captured in November by the robotic Cassini spacecraft in orbit around Saturn as it swooped past the giant ice ball. Cassini has now started on its Grand Finale Tour which will take it inside Saturn's rings and culminate in September with a dive into Saturn's thick atmosphere.",https://apod.nasa.gov/apod/image/1702/Tethys_Cassini_1020.jpg,image,v1,Odysseus Crater on Tethys,https://apod.nasa.gov/apod/image/1702/Tethys_Cassini_960.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2019-04-26,"Tracking along the southern Milky Way this beautiful celestial mosaic was recorded under dark Brazilian skies. Spanning some 20 degrees it actually starts with the dark expanse of the Coalsack nebula at the lower left, tucked under an arm of the Southern Cross. That compact constellation is topped by bright yellowish Gamma Crucis, a cool giant star a mere 88 light-years distant. A line from Gamma Crucis through the blue star at the bottom of the cross, Alpha Crucis, points toward the South Celestial Pole. Follow the Milky Way to the right and your gaze will sweep across IC 2948, popularly known as the Running Chicken nebula, before it reaches Eta Carinae and the Carina Nebula near the right edge of the frame. About 200 light-years across, the Carina Nebula is a star forming region much larger than the more northerly stellar nursery the Orion Nebula. The Carina Nebula lies around 7,500 light-years from Earth along the plane of the Milky Way.",https://apod.nasa.gov/apod/image/1904/FairbairnCROSSTOCARINA1024.jpg,image,v1,Southern Cross to Eta Carinae,https://apod.nasa.gov/apod/image/1904/FairbairnCROSSTOCARINA.jpg,Carlos Fairbairn,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2008-04-26,"The Tarantula Nebula is more than 1,000 light-years in diameter -- a giant star forming region within our neighboring galaxy the Large Magellanic Cloud (LMC). That cosmic arachnid lies at the upper left of this expansive mosiac covering a part of the LMC over 6,000 light-years across. 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 violent star-forming regions with young star clusters, filaments and bubble-shaped clouds. The small but expanding remnant of supernova 1987a, the closest supernova in modern history, is located near the center of the view. The rich field is about as wide as four full moons on the sky, located in the southern constellation Dorado.",https://apod.nasa.gov/apod/image/0804/Tarantulamosaic_gendler.jpg,image,v1,The Tarantula Zone,https://apod.nasa.gov/apod/image/0804/Tarantulamosaic_gendler800.jpg,Robert Gendler,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2002-12-29,"Globular clusters once ruled the Milky Way. Back in the old days, back when our Galaxy first formed, perhaps thousands of globular clusters roamed our Galaxy. Today, there are perhaps 200 left. Many globular clusters were destroyed over the eons by repeated fateful encounters with each other or the Galactic center. Surviving relics are older than any Earth fossil, older than any other structures in our Galaxy, and limit the universe itself in raw age. There are few, if any, young globular clusters in our Milky Way Galaxy because conditions are not ripe for more to form. Things are different next door, however, in the neighboring LMC galaxy. Pictured above is a ""young"" globular cluster residing there: NGC 1818. Observations show it formed only about 40 million years ago - just yesterday compared to the 12 billion year ages of globular clusters in our own Milky Way",https://apod.nasa.gov/apod/image/0103/ngc1818_hst_big.jpg,image,v1,NGC 1818: A Young Globular Cluster,https://apod.nasa.gov/apod/image/0103/ngc1818_hst.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2001-09-09,"Hot blue stars shine brightly in this beautiful, recently formed galactic or ""open"" star cluster. Open cluster NGC 3293 is located in the constellation Carina, lies at a distance of about 8000 light years, and has a particularly high abundance of these young bright stars. A study of NGC 3293 implies that the blue stars are only about 6 million years old, whereas the cluster's dimmer, redder stars appear to be about 20 million years old. If true, star formation in this open cluster took at least 15 million years. Even this amount of time is short, however, when compared with the billions of years stars like our Sun live, and the over-ten billion year lifetimes of many galaxies and our universe. NGC 3293 appears just in front of a dense dust lane emanating from the Carina Nebula.",https://apod.nasa.gov/apod/image/0109/ngc3293_aao.jpg,image,v1,NGC 3293: A Bright Young Open Cluster,https://apod.nasa.gov/apod/image/0109/ngc3293_aao_big.jpg,AAO,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -1997-09-05,"Twenty five years ago humans roamed the Moon. Pictured here during the last moon landing, scientist-astronaut Harrison Schmitt was photographed standing next to a huge, split boulder. Apollo 17 was one of six missions that landed humans on the moon and returned them safely. Apollo 17 explored the unusually dark terrain at the Taurus-Littrow landing site, deployed explosives to test the internal geology of the Moon, and returned the most rocks of any lunar mission.",https://apod.nasa.gov/apod/image/9709/boulder_a17_big.jpg,image,v1,Apollo 17: Boulder on the Moon,https://apod.nasa.gov/apod/image/9709/boulder_a17.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -1997-06-09,"Do other planets have aurora? Terrestrial and spacecraft observations have found evidence for aurora on Venus, Mars, Jupiter, Saturn, Uranus, and Neptune. In the above false-color photograph, a good portion of an auroral ring was captured recently in optical light by the Galileo spacecraft in orbit around Jupiter. Auroral rings encircle a planet's magnetic pole, and result from charged particles spiraling down magnetic field lines. Although the surroundings near Jupiter are much different than Earth, the auroral rings appear similar.",https://apod.nasa.gov/apod/image/9706/jup_aring_big.jpg,image,v1,An Auroral Ring on Jupiter,https://apod.nasa.gov/apod/image/9706/jup_aring.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2015-01-31,"Infrared wavelengths of 3.6, 8.0, and 24.0 microns observed by the Spitzer Space Telescope are mapped into visible colors red, green, and blue in this striking image. The cosmic cloud of gas and dust is W33, a massive starforming complex some 13,000 light-years distant, near the plane of our Milky Way Galaxy. So what are all those yellow balls? Citizen scientists of the web-based Milky Way Project found the features they called yellow balls as they scanned many Spitzer images and persistently asked that question of researchers. Now there is an answer. The yellow balls in Spitzer images are identified as an early stage of massive star formation. They appear yellow because they are overlapping regions of red and green, the assigned colors that correspond to dust and organic molecules known as PAHs at Spitzer wavelengths. Yellow balls represent the stage before newborn massive stars clear out cavities in their surrounding gas and dust and appear as green-rimmed bubbles with red centers in the Spitzer image. Of course, the astronomical crowdsourcing success story is only part of the Zooniverse. The Spitzer image spans 0.5 degrees or about 100 light-years at the estimated distance of W33.",https://apod.nasa.gov/apod/image/1501/sig15-02spitzerW33.jpg,image,v1,Yellow Balls in W33,https://apod.nasa.gov/apod/image/1501/sig15-02spitzerW331066.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2000-04-03,"A huge eruptive prominence is seen moving out from our Sun in this condensed half-hour time-lapse sequence. Ten Earths could easily fit in the ""claw"" of this seemingly solar monster. This large prominence, though, is significant not only for its size, but its shape. The twisted figure eight shape indicates that a complex magnetic field threads through the emerging solar particles. Recent evidence of differential rotation inside the Sun might help account for the surface explosion. The sequence was taken early this year by the Sun-orbiting SOHO satellite. Although large prominences and energetic Coronal Mass Ejections (CMEs) are relatively rare, they are occurring more frequently now that we are near the Solar Maximum, a time of peak sunspot and solar activity in the eleven-year solar cycle.",https://apod.nasa.gov/apod/image/0004/prom1743_eit_big.gif,image,v1,A Twisted Solar Eruptive Prominence,https://apod.nasa.gov/apod/image/0004/promanim3_eit.gif,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2013-03-29,"Orbiting in the plane of Saturn's rings, Saturnian moons have a perpetual ringside view of the gas giant planet. Of course, while passing near the ring plane the Cassini spacecraft also shares their stunning perspective. The thin rings themselves slice across the middle of this Cassini snapshot from April 2011. The scene looks toward the dark night side of Saturn, in the frame at the left, and the still sunlit side of the rings from just above the ringplane. Centered, over 1,500 kilometers across, Rhea is Saturn's second largest moon and is closest to the spacecraft, around 2.2 million kilometers away. To Rhea's right, shiny, 500 kilometer diameter Enceladus is about 3 million kilometers distant. Dione, 1,100 kilometers wide, is 3.1 million kilometers from Cassini's camera on the left, partly blocked by Saturn's night side.",https://apod.nasa.gov/apod/image/1303/PIA12771.jpg,image,v1,Ringside with Rhea,https://apod.nasa.gov/apod/image/1303/PIA12771_c900.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2015-05-25,"First came the trees. In the town of Salamanca, Spain, the photographer noticed how distinctive a grove of oak trees looked after being pruned. Next came the galaxy. The photographer stayed up until 2 am, waiting until the Milky Way Galaxy rose above the level of a majestic looking oak. From this carefully chosen perspective, dust lanes in the galaxy appear to be natural continuations to branches of the tree. Last came the light. A flashlight was used on the far side of the tree to project a silhouette. By coincidence, other trees also appeared as similar silhouettes across the relatively bright horizon. The featured image was captured as a single 30-second frame earlier this month and processed to digitally enhance the Milky Way.",https://apod.nasa.gov/apod/image/1505/MWTree_Toledano_6016.jpg,image,v1,The Galaxy Tree,https://apod.nasa.gov/apod/image/1505/MWTree_Toledano_1080.jpg," -C�sar Vega Toledano ; - Rollover Annotation: Judy Schmidt -",exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2016-01-24,"In the center of star-forming region 30 Doradus lies a huge cluster containing some of the largest, hottest, and most massive stars known. These stars, known collectively as star cluster R136, were captured in the featured image in visible light by the Wide Field Camera 3 in 2009 peering through the Hubble Space Telescope. Gas and dust clouds in 30 Doradus, also known as the Tarantula Nebula, have been sculpted into elongated shapes by powerful winds and ultraviolet radiation from these hot cluster stars. The 30 Doradus Nebula lies within a neighboring galaxy known as the Large Magellanic Cloud and is located a mere 170,000 light-years away.",https://apod.nasa.gov/apod/image/1601/30dor_hubble_3939.jpg,image,v1,Star Cluster R136 Bursts Out,https://apod.nasa.gov/apod/image/1601/30dor_hubble_960.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2017-01-09,"What's happening in the center of spiral NGC 5033? Many things -- some circular, some energetic, and some not well understood. NGC 5033 is known as a Seyfert galaxy because of the great activity seen in its nucleus. Bright stars, dark dust, and interstellar gas all swirl quickly around a galactic center that appears slightly offset from a supermassive black hole. This offset is thought to be the result of NGC 5033 merging with another galaxy sometime in the past billion years. The featured image was taken by the Hubble Space Telescope in 2005. NGC 5033 spans about 100,000 light years and is so far away that we see it only as it existed about 40 million years ago.",https://apod.nasa.gov/apod/image/1701/NGC5033_HubbleSchmidt_1280.jpg,image,v1,In the Center of Spiral Galaxy NGC 5033,https://apod.nasa.gov/apod/image/1701/NGC5033_HubbleSchmidt_960.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2021-08-04,"How do supermassive black holes create powerful jets? To help find out, the Event Horizon Telescope (EHT) imaged the center of the nearby active galaxy Centaurus A. The cascade of featured inset images shows Cen A from it largest, taking up more sky than many moons, to its now finest, taking up only as much sky as an golf ball on the moon. The new image shows what may look like two jets -- but is actually two sides of a single jet. This newly discovered jet-edge brightening does not solve the jet-creation mystery, but does imply that the particle outflow is confined by a strong pressure -- possibly involving a magnetic field. The EHT is a coordination of radio telescopes from around the Earth -- from the Caltech Submillimeter Observatory in Hawaii USA, to ALMA in Chile, to NOEMA in France, and more. The EHT will continue to observe massive, nearby black holes and their energetic surroundings.",https://apod.nasa.gov/apod/image/2108/CenAjets_Eht_3001.jpg,image,v1,EHT Resolves Central Jet from Black Hole in Cen A,https://apod.nasa.gov/apod/image/2108/CenAjets_Eht_960.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2004-03-10,"How prevalent was water on Mars? Results from the Spirit rover now indicate that Gusev crater likely had a wet past, a result that comes shortly after Spirit's twin rover Opportunity uncovered clear evidence of past water at Meridiani Planum on the other side of Mars. Evidence uncovered by Spirit and released last week focussed on a large rock of unusual shape nicknamed Humphrey, shown above near the image bottom. Detailed inspection of the rock revealed a bright material filling internal cracks. Such material may have crystallized from water trickling through the volcanic rock. The amount of Mars once covered by ancient water remains unknown, as both rovers landed in regions thought likely to once be underwater. Spirit continues to roll across Mars, recently passing the 300-meter mark on its way to Bonneville crater.",https://apod.nasa.gov/apod/image/0403/humphrey_spirit_big.jpg,image,v1,Humphrey Rock Indicates Ancient Martian Water,https://apod.nasa.gov/apod/image/0403/humphrey_spirit.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2018-07-25,"What kind of celestial object is this? A relatively normal galaxy -- but seen from its edge. Many disk galaxies are actually just as thin as NGC 5866, pictured here, but are not seen edge-on from our vantage point. A perhaps more familiar galaxy seen edge-on is our own Milky Way Galaxy. Cataloged as M102 and NGC 5866, the Spindle galaxy has numerous and complex dust lanes appearing dark and red, while many of the bright stars in the disk give it a more blue underlying hue. The blue disk of young stars can be seen extending past the dust in the extremely thin galactic plane. There is evidence that the Spindle galaxy has cannibalized smaller galaxies over the past billion years or so, including multiple streams of faint stars, dark dust that extends away from the main galactic plane, and a surrounding group of galaxies (not shown). In general, many disk galaxies become thin because the gas that forms them collides with itself as it rotates about the gravitational center. The Spindle galaxy lies about 50 million light years distant toward the constellation of the Dragon (Draco).",https://apod.nasa.gov/apod/image/1807/NGC5866_Block_1518.jpg,image,v1,The Edge-On Spindle Galaxy,https://apod.nasa.gov/apod/image/1807/NGC5866_Block_960.jpg,Adam Block,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2009-07-27,"What's happening at the center of spiral galaxy NGC 1097? No one is sure, but it likely involves a supermassive black hole. Matter falling in from a bar of stars and gas across the center is likely being heated by an extremely energetic region surrounding the central black hole. From afar, the entire central region appears in the above false-color infrared image as a mysterious eye. Near the left edge and seen in blue, a smaller companion galaxy is wrapped in the spectacular spiral arms of the large spiral, lit in pink by glowing dust. Currently about 40 thousand light-years from the larger galaxy's center, the gravity of the companion galaxy appears to be reshaping the larger galaxy as it is slowly being destroyed itself. NGC 1097 is located about 50 million light years away toward the constellation of the furnace (Fornax). Note: An APOD editor will review great space images this Saturday night at Ft. Wilkins, Michigan.",https://apod.nasa.gov/apod/image/0907/ngc1097_spitzer_big.jpg,image,v1,NGC 1097: Spiral Galaxy with a Central Eye,https://apod.nasa.gov/apod/image/0907/ngc1097_spitzer.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2016-07-09,"Bright noctilucent or night shining clouds are not familiar sights from northern France. But these electric-blue waves coursed through skies over the small town of Wancourt in Pas-de-Calais on July 6, just before the dawn. From the edge of space, about 80 kilometers above Earth's surface, the icy clouds still reflect sunlight even though the Sun itself is below the horizon as seen from the ground. Usually spotted at high latitudes in summer months the diaphanous apparitions are also known as polar mesospheric clouds. The seasonal clouds are understood to form as water vapor driven into the cold upper atmosphere condenses on the fine dust particles supplied by disintegrating meteors or volcanic ash. NASA's AIM mission provides projections of the noctilucent clouds as seen from space.",https://apod.nasa.gov/apod/image/1607/Lericque-Simon-nlc06072016-3-ok_1467777140.jpg,image,v1,Noctilucent Clouds Tour France,https://apod.nasa.gov/apod/image/1607/Lericque-Simon-nlc06072016-3-ok_1467777140_1152c.jpg,GAAC,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2020-04-14,"NGC 253 is one of the brightest spiral galaxies visible, but also one of the dustiest. Dubbed the Silver Coin for its appearance in smalltelescopes, it is more formally known as the Sculptor Galaxy for its location within the boundaries of the southern constellation Sculptor. Discovered in 1783 by mathematician and astronomer Caroline Herschel, the dusty island universe lies a mere 10 million light-years away. About 70 thousand light-years across, NGC 253, pictured, is the largest member of the Sculptor Group of Galaxies, the nearest to our own Local Group of galaxies. In addition to its spiral dust lanes, tendrils of dust seem to be rising from a galactic disk laced with young star clusters and star forming regions in this sharp color image. The high dust content accompanies frantic star formation, earning NGC 253 the designation of a starburst galaxy. NGC 253 is also known to be a strong source of high-energy x-rays and gamma rays, likely due to massive black holes near the galaxy's center. Take a trip through extragalactic space in this short video flyby of NGC 253. Astrophysicists: Browse 2,100+ codes in the Astrophysics Source Code Library",https://apod.nasa.gov/apod/image/2004/NGC253_HstSubaruEsoNew_3500.jpg,image,v1,NGC 253: The Silver Coin Galaxy,https://apod.nasa.gov/apod/image/2004/NGC253_HstSubaruEsoNew_960.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2014-01-21,"Did you see the big, bright, beautiful Full Moon last Wednesday night? That was actually a Micro Moon! On that night, the smallest Full Moon of 2014 reached its full phase only a few hours from lunar apogee, the time of its the most distant point from Earth in the Moon's elliptical orbit. Of course, last year on the night of June 22, a Full Super Moon was near perigee, the closest point in its orbit. The relative apparent size of January 15's Micro Moon is compared to the June 22 Super Moon in the above composite image digitally superimposing telescopic images from Perugia, Italy. The difference in apparent size represents a difference in distance of just under 50,000 kilometers between apogee and perigee, given the Moon's average distance of about 385,000 kilometers. How long do you have to wait to see another Full Micro Moon? Until March 5, 2015, when the lunar full phase will again occur within a few hours of lunar apogee.",https://apod.nasa.gov/apod/image/1401/microsupermoon_sciarpetti_459.jpg,image,v1,Micro Moon over Super Moon,https://apod.nasa.gov/apod/image/1401/microsupermoon_sciarpetti_960.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -1997-01-02,"What caused the bubbles and arcs in NGC 2359? The main suspect is the Wolf-Rayet star in the center of one of the bubbles - visible slightly below and to the right of the center of the above photograph. Most Wolf-Rayet stars are known to be massive, highly luminous stars that continually cast off material in a stellar wind - which commonly form bubbles in the interstellar medium. But the unusual structure of the NGC 2359 arcs indicate something more complex is going on. Is the star moving supersonically? Is there another energetic star in the vicinity? Future observations may give more pieces to this picturesque puzzle. ",https://apod.nasa.gov/apod/image/9701/ngc2359_cfa_big.jpg,image,v1,Bubbles and Arcs in NGC 2359,https://apod.nasa.gov/apod/image/9701/ngc2359_cfa.jpg,"P. Berlind & P. Challis -(CfA), 1.2-m Telescope, -Whipple Obs.",exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -1998-11-13,"This bright fireball meteor was photographed from Table Mountain Observatory during the peak of the annual Leonid meteor shower on November 17, 1966. That was a good year for Leonid meteor watchers - a meteor ""storm"" was produced as the Earth swept through a dense swarm of dusty debris from the tail of comet Tempel-Tuttle. Observer Jim Young reported a peak rate for the 1966 shower of about 50 meteors per second and recorded 22 otherwise extremely rare, bright fireballs like this one in the span of 90 minutes from his California mountain top location. Predictions are uncertain, but this year might also produce an intense apparition of the Leonids shower which should again peak on the 17th. You may need to be well placed and a little lucky to see the shower at its maximum, but Leonid meteors should be easy to see in dark skies - particularly in early morning hours - for two or so days before and after the peak. How do you watch a meteor shower? Get a comfortable lawn chair and a warm jacket ... go outside and look up!",https://apod.nasa.gov/apod/image/9811/leonidfball66_young_big.jpg,image,v1,A Leonid Fireball From 1966,https://apod.nasa.gov/apod/image/9811/leonidfball66_young.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2014-04-23,"From planet Earth, we see this strongly distorted pair of galaxies, cataloged as Arp 81, as they were only about 100 million years after their close encounter. The havoc wreaked by their mutual gravitational interaction during the encounter is detailed in this color composite showing twisted streams of gas and dust, a chaos of massive star formation, and a tidal tail stretching for 200 thousand light-years or so as it sweeps behind the cosmic wreckage. Also known as NGC 6622 (left) and NGC 6621, the galaxies are roughly equal in size but are destined to merge into one large galaxy in the distant future, making repeated approaches until they finally coalesce. Located in the constellation Draco, the galaxies are 280 million light-years away. Even more distant background galaxies can be spotted in the sharp, reprocessed, image from Hubble Legacy Archive data.",https://apod.nasa.gov/apod/image/1404/ARP81_HLA_Pugh2.jpg,image,v1,Arp 81: 100 Million Years Later,https://apod.nasa.gov/apod/image/1404/ARP81_HLA_Pugh2.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2018-10-06,"What does an aurora look like to a frog? ""Awesome!"" is the likely answer, suggested by this imaginative snapshot taken on October 3rd from Kiruna, Sweden. Frequented by apparitions of the northern lights, Kiruna is located in Lapland north of the Arctic Circle, and often under the auroral oval surrounding planet Earth's geomagnetic north pole. To create a tantalizing view from a frog's perspective the photographer turned on the flashlight on her phone and placed it on the ground facing down, resting her camera's lens on top. The ""diamonds"" in the foreground are icy pebbles right in front of the lens, lit up by the flashlight. Reflecting the shimmering northern lights, the ""lake"" is a frozen puddle on the ground. Of course, in the distance is the Bengt Hultqvist Observatory.",https://apod.nasa.gov/apod/image/1810/AuroraFrogStalnacke3072.jpg,image,v1,Aurora: The Frog's View,https://apod.nasa.gov/apod/image/1810/AuroraFrogStalnacke1024.jpg,Mia Stalnacke,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2019-12-19,"Awkward and angular looking, Apollo 17's lunar module Challenger was designed for flight in the near vacuum of space. Digitally enhanced and reprocessed, this picture taken from Apollo 17's command module America shows Challenger's ascent stage in lunar orbit. Small reaction control thrusters are at the sides of the moonship with the bell of the ascent rocket engine underneath. The hatch allowing access to the lunar surface is seen at the front, with a round radar antenna at the top. Mission commander Gene Cernan is clearly visible through the triangular window. This spaceship performed gracefully, landing on the Moon and returning the Apollo astronauts to the orbiting command module in December of 1972. So where is Challenger now? Its descent stage remains at the Apollo 17 landing site in the Taurus-Littrow valley. The ascent stage pictured was intentionally crashed nearby after being jettisoned from the command module prior to the astronauts' return to planet Earth. Apollo 17's mission came to an end 47 years ago today. It was the sixth and last time astronauts landed on the Moon.",https://apod.nasa.gov/apod/image/1912/AS17-149-22859-2v2SmlWmk.jpg,image,v1,Apollo 17's Moonship,https://apod.nasa.gov/apod/image/1912/AS17-149-22859-2v2SmlWmk1024.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -1997-09-13,"Johannes Kepler used simple mathematics to describe how planets move. Kepler was an assistant to the most accurate astronomical observer of the time, Tycho Brahe. Kepler was able to use Brahe's data to show that planets move in ellipses around the Sun (Kepler's First Law), that planets move proportionally faster in their orbits when they are nearer the Sun (Kepler's Second Law), and that more distant planets take proportionally longer to orbit the Sun (Kepler's Third Law). Kepler lived from 1571 to 1630, during the time of discovery of the telescope. Kepler was one of the few vocal supporters of Galileo's discoveries and the Copernican system of planets orbiting the Sun instead of the Earth.",https://apod.nasa.gov/apod/image/kepler_hist_big.gif,image,v1,Kepler Discovers How Planets Move,https://apod.nasa.gov/apod/image/kepler_hist.gif,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2020-07-15,"Comet NEOWISE has been wowing photographers around much of the world during dawn and dusk, at the margins of day and night. For the most northern residents of planet Earth, however, the comet circles the North Star and never sets. The night part of this circular arc is apparent in the featured composite of images assembled from a webcam located at a ski resort in the Swiss Alps. Images were selected at 30-minute intervals throughout the night from July 12th -13th. Comet NEOWISE (C/2020 F3) will continue to become more accessible to northern hemisphere observers as its motion places it higher in the sky each evening after sunset over the next few weeks, as it begins its outbound journey. As with all comets, departure from the inner Solar System comes with inevitable fading. Binoculars are the best way to find and observe the comet visually. Notable Images of Comet NEOWISE Submitted to APOD: || July 14 || July 13 || July 12 || July 11 || July 10 & earlier ||",https://apod.nasa.gov/apod/image/2007/NeowiseAlps_salzgeber_4000.jpg,image,v1,Comet NEOWISE over the Swiss Alps,https://apod.nasa.gov/apod/image/2007/NeowiseAlps_salzgeber_960.jpg," -Philipp Salzgeber, -foto-webcam.eu; -Text: -Adam Block -",exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2009-08-19,"Sprawling across hundreds of light-years, emission nebula IC 1396, visible on the upper right, mixes glowing cosmic gas and dark dust clouds. Stars are forming in this area, only about 3,000 light-years from Earth. This wide angle view also captures surrounding emission and absorption nebula. The red glow in IC 1396 and across the image is created by cosmic hydrogen gas recapturing electrons knocked away by energetic starlight. The dark dust clouds are dense groups of smoke-like particles common in the disks of spiral galaxies. Among the intriguing dark shapes within IC 1396, the winding Elephant's Trunk nebula lies just right of the nebula's center. IC 1396 lies in the high and far off constellation of Cepheus.",https://apod.nasa.gov/apod/image/0908/ic1396_earle_big.jpg,image,v1,IC 1396 and Surrounding Starfield,https://apod.nasa.gov/apod/image/0908/ic1396_earle.jpg,Thomas W. Earle,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -1999-03-08,Tomorrow's picture: The VLT Interferometric Array < 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/9903/jvconjunction_polakis_big.jpg,image,v1,A Jupiter Venus Conjunction,https://apod.nasa.gov/apod/image/9903/jvconjunction_polakis.jpg," -T. Polakis -",exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2004-10-27,"Go outside tonight and see the total lunar eclipse. Tonight's eclipse is easy and convenient for much of the world to see. Anyone who can spot a full Moon can see it fade out as the Earth's shadow engulfs it. No protective glasses or expensive telescopes are needed, just a little moxie. The above illustration shows how the eclipse will appear across the Earth. The total lunar eclipse starts at 9:14 pm Eastern Daylight Time, equivalent to 1:14 am UT in the morning for sky enthusiasts in the United Kingdom. From the moment the first part of the Moon disappears to the moment that the last part of the Moon reappears will be 3 hours and 40 minutes. For those unfortunate enough to suffer clouds, the eclipse can also be followed over several live webcasts. World Series Lunar Eclipse: Live TV shot makes this eclipse possibly the most seen live eclipse ever.",https://apod.nasa.gov/apod/image/0410/lunareclipse041028_nasa_big.gif,image,v1,Total Lunar Eclipse Tonight,https://apod.nasa.gov/apod/image/0410/lunareclipse041028_nasa.gif,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2002-07-06,"How big is the Jovian moon Io? The most volcanic body in the Solar System, Io (usually pronounced ""EYE-oh"") is 3,600 kilometers in diameter, about the size of planet Earth's single large natural satellite. Gliding past Jupiter at the turn of the millennium, the Cassini spacecraft captured this awe inspiring view of active Io with the largest gas giant as a backdrop, offering a stunning demonstration of the ruling planet's relative size. Although in the picture Io appears to be located just in front of the swirling Jovian clouds, Io hurtles around its orbit once every 42 hours at a distance of 420,000 kilometers or so from the center of Jupiter. That puts it nearly 350,000 kilometers above Jupiter's cloud tops, roughly equivalent to the distance between Earth and Moon. The Cassini spacecraft itself was about 10 million kilometers from Jupiter when recording the image data.",https://apod.nasa.gov/apod/image/0207/iojup_cassini_big.jpg,image,v1,Io: Moon Over Jupiter,https://apod.nasa.gov/apod/image/0207/iojup_cassini.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2013-09-22,"Today, the Sun crosses the celestial equator heading south at 20:44 Universal Time. An equinox (equal night), this astronomical event marks the first day of autumn in the northern hemisphere and spring in the south. With the Sun on the celestial equator, Earth dwellers will experience nearly 12 hours of daylight and 12 hours of darkness. To celebrate, consider this remarkable record of the Sun's yearly journey through planet Earth's sky, made with planned multiple exposures captured on a single piece of 35 millimeter film. Exposures were made at the same time of day (9:00am local time), capturing the Sun's position on dates from January 7 through December 20, 2003. The multiple suns trace an intersecting curve known as an analemma. A foreground base exposure of the Temple of Apollo in ancient Corinth, Greece, appropriate for an analemma, was digitally merged with the film image. Equinox dates correspond to the middle points (not the intersection point) of the analemma. The curve is oriented at the corresponding direction and altitude for the temple, so the Sun's position for the September equinox is at the upper midpoint near picture center. Summer and winter solstices are at analemma top and bottom.",https://apod.nasa.gov/apod/image/1309/solar-analemma-070000-900pix.jpg,image,v1,Apollo's Analemma,https://apod.nasa.gov/apod/image/1309/solar-analemma-070000-900pix.jpg,Anthony Ayiomamitis,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2000-06-19,"A jet stretching nearly a million light years has been imaged emanating from galaxy Pictor A. The thin jet of electrons and protons shoots out at nearly light-speed likely from the vicinity of a large black hole at the galaxy center. At the left of the above image in X-rays is the radio galaxy Pictor A, known as a radio galaxy for its strong radio emission. At the far end of the jet on the right a hot spot glows as the intense particle beam bores through a gas cloud in intergalactic space. The jet and hot spot of Pictor A had been seen previously in radio waves, but only recently has the orbiting Chandra X-ray Observatory confirmed its unusual power.",https://apod.nasa.gov/apod/image/0006/pictora_chandra_big.jpg,image,v1,The Long Jet of Pictor A,https://apod.nasa.gov/apod/image/0006/pictora_chandra.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2017-06-08,"On certain dates in February, an elusive firefall can be spotted at sunset in Yosemite National Park, when the weather cooperates and the direction to the setting Sun is just right. Often photographed from vantage points below, at the right moment the park's seasonal Horsetail Fall is isolated in the shadows of the steep walls of El Capitan. Then, still illuminated with rays of sunlight reflected by the angled rockface directly behind the flow, the waterfall briefly takes on a dramatic, fiery appearance. The Horsetail firefall is more rarely photographed at moonset under a starry night sky, though. Even more elusive by moonlight, the firefall effect can also be seen when skies are clear and a bright Moon sets at the right direction along the western horizon. Skies were clear and stars were shining for this well-planned photograph of the Horsetail firefall lit by a gibbous Moon setting in the early morning hours of May 9.",https://apod.nasa.gov/apod/image/1706/MLFirefall_WF2_960.jpg,image,v1,Firefall by Moonlight,https://apod.nasa.gov/apod/image/1706/MLFirefall_WF2_960.jpg,"Rogelio Bernal -Andreo",exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2018-09-02,"It was one of the most powerful solar flares in recorded history. Occurring in 2003 and seen across the electromagnetic spectrum, the Sun briefly became over 100 times brighter in X-rays than normal. The day after this tremendous X 17 solar flare -- and subsequent Coronal Mass Ejection (CME) -- energetic particles emitted from the explosions struck the Earth, creating auroras and affecting satellites. The spacecraft that took these frames -- SOHO -- was put in a turtle-like safe mode to avoid further damage from this and subsequent solar particle storms. The featured time-lapse movie condenses into 10 seconds events that occurred over 4 hours. The CME, visible around the central sun-shade, appears about three-quarters of the way through the video, while frames toward the very end are progressively noisier as protons from the explosions strike SOHO's LASCO detector. One this day in 1859, the effects of an even more powerful solar storm caused telegraphs on Earth to spark in what is known as the Carrington Event. Powerful solar storms such as these may create beautiful aurora-filled skies, but they also pose a real danger as they can damage satellites and even power grids across the Earth.",,video,v1,A Powerful Solar Flare,https://www.youtube.com/embed/vzh7udgtDKA?rel=0,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2010-06-03,"SOFIA, the Stratospheric Observatory for Infrared Astronomy, captured its ""first light"" images on May 26, from an altitude of 35,000 feet. While flying above most of planet Earth's infrared-absorbing water vapor, SOFIA's premier infrared views of the cosmos included this remarkable false-color image (right panel) of Jupiter. For comparison, on the left is a recent, ground-based visible light image. Both show our solar system's ruling gas giant without its dark southern equatorial belt (normally seen in the upper hemisphere in this orientation). That familiar feature faded from view early in May. But the bright white stripe in SOFIA's image is a region of Jupiter's clouds transparent to infrared light, offering a glimpse below the cloud tops.",https://apod.nasa.gov/apod/image/1006/Jupiter_sofiawesley.jpg,image,v1,Jupiter from the Stratosphere,https://apod.nasa.gov/apod/image/1006/Jupiter_sofiawesley900c.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2016-02-11,"Gravitational radiation has been directly detected. The first-ever detection was made by both facilities of the Laser Interferometer Gravitational-Wave Observatory (LIGO) in Washington and Louisiana simultaneously last September. After numerous consistency checks, the resulting 5-sigma discovery was published today. The measured gravitational waves match those expected from two large black holes merging after a death spiral in a distant galaxy, with the resulting new black hole momentarily vibrating in a rapid ringdown. A phenomenon predicted by Einstein, the historic discovery confirms a cornerstone of humanity's understanding of gravity and basic physics. It is also the most direct detection of black holes ever. The featured illustration depicts the two merging black holes with the signal strength of the two detectors over 0.3 seconds superimposed across the bottom. Expected future detections by Advanced LIGO and other gravitational wave detectors may not only confirm the spectacular nature of this measurement but hold tremendous promise of giving humanity a new way to see and explore our universe.",https://apod.nasa.gov/apod/image/1602/BHmerger_LIGO_3600.jpg,image,v1,LIGO Detects Gravitational Waves from Merging Black Holes,https://apod.nasa.gov/apod/image/1602/BHmerger_LIGO_960.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -1996-07-01,"Within the last few years, observational astronomy has given humanity evidence of the existence of worlds beyond the solar system. Indeed, solar-type stars are now inferred to harbor planets of approximately Jupiter mass - some residing in temperature zones which could conceivably support liquid water and therefore life! Above is a hypothetical scene near one such planet whose sun, 47 Ursae Majoris (47 UMa), is a yellow dwarf star (spectral class G0 V) very similar to our own. In our sky, it appears as a faint, inconspicuous star below the cup of the northern hemisphere asterism, ""the Big Dipper"". (Our own sun would be equally inconspicuous when viewed from 47 UMa ...) Astronomer's G. Marcy and P. Butler announced the discovery of a planet associated with this star in 1996 and reported it to have a mass of about 2.4 Jupiters or more with an orbital period of 3 years. This artist's vision pictures the detected planet, referred to as 47 UMa b, as a gas giant surrounded by a ring of material - analogous to our own gas giant Saturn. In the foreground lies a hypothetical moon of 47 UMa b. Could such a moon support life? 47 UMa is only 44 light years distant, fairly close by astronomical standards - yet there is evidence for planetary systems which are closer still. NASA plans to explore nearby planetary systems using spaceborne observatories. APOD News: RJN to MTU",https://apod.nasa.gov/apod/image/whatm_47uma1_big.jpg,image,v1,Worlds of a Distant Sun: 47 Ursae Majoris b,https://apod.nasa.gov/apod/image/whatm_47uma1.gif," -John Whatmough, -Extrasolar Visions -",exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2018-09-09,"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 featured 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/1809/CrabNebula_Hubble_3864.jpg,image,v1,M1: The Crab Nebula from Hubble,https://apod.nasa.gov/apod/image/1809/CrabNebula_Hubble_960.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2008-04-28,"What's happening in the NGC 3582 nebula? Bright stars and interesting molecules are forming. The complex nebula resides in the star forming region called RCW 57. Visible in this image are dense knots of dark interstellar dust, bright stars that have formed in the past few million years, fields of glowing hydrogen gas ionized by these stars, and great loops of gas expelled by dying stars. A recent detailed study of NGC 3582 uncovered at least 33 massive stars in the end stages of formation, and the clear presence of the complex carbon molecules known as polycyclic aromatic hydrocarbons (PAHs). PAHs are thought to be created in the cooling gas of star forming regions, and their development in the Sun's formation nebula five billion years ago may have been an important step in the development of life on Earth. This picture was taken last year with the Blanco 4-meter telescope at the Cerro Tololo Inter-American Observatory (CTIO), in Chile.",https://apod.nasa.gov/apod/image/0804/ngc3582_noao_big.jpg,image,v1,Star Forming Region NGC 3582,https://apod.nasa.gov/apod/image/0804/ngc3582_noao.jpg,T. A. Rector,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2019-09-20,"Still bright in planet Earth's night skies, good telescopic views of Saturn and its beautiful rings often make it a star at star parties. But this stunning view of Saturn's rings and night side just isn't possible from telescopes closer to the Sun than the outer planet. They can only bring Saturn's day into view. In fact, this image of Saturn's slender sunlit crescent with night's shadow cast across its broad and complex ring system was captured by the Cassini spacecraft. A robot spacecraft from planet Earth, Cassini called Saturn orbit home for 13 years before it was directed to dive into the atmosphere of the gas giant on September 15, 2017. This magnificent mosaic is composed of frames recorded by Cassini's wide-angle camera only two days before its grand final plunge. Saturn's night will not be seen again until another spaceship from Earth calls.",https://apod.nasa.gov/apod/image/1909/LastRingPortrait_Cassini_4472.jpg,image,v1,Saturn at Night,https://apod.nasa.gov/apod/image/1909/LastRingPortrait_Cassini_1080.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2013-05-19,"What on Earth is that? The Richat Structure in the Sahara Desert of Mauritania is easily visible from space because it is nearly 50 kilometers across. Once thought to be an impact crater, the Richat Structure's flat middle and lack of shock-altered rock indicates otherwise. The possibility that the Richat Structure was formed by a volcanic eruption also seems improbable because of the lack of a dome of igneous or volcanic rock. Rather, the layered sedimentary rock of the Richat structure is now thought by many to have been caused by uplifted rock sculpted by erosion. The above image was captured by the ASTER instruments onboard the orbiting orbiting Terra satellite. Why the Richat Structure is nearly circular remains a mystery.",https://apod.nasa.gov/apod/image/1305/richat_aster_3130.jpg,image,v1,Earth's Richat Structure,https://apod.nasa.gov/apod/image/1305/richat_aster_960.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2012-10-07,"Are square A and B the same color? They are! To verify this, either run your cursor over the image or click here to see them connected. The above illusion, called the same color illusion, illustrates that purely human observations in science may be ambiguous or inaccurate. Even such a seemingly direct perception as relative color. Similar illusions exist on the sky, such as the size of the Moon near the horizon, or the apparent shapes of astronomical objects. The advent of automated, reproducible, measuring devices such as CCDs have made science in general and astronomy in particular less prone to, but not free of, human-biased illusions.",https://apod.nasa.gov/apod/image/1210/greyillusion_wikipedia_960.jpg,image,v1,The Same Color Illusion,https://apod.nasa.gov/apod/image/1210/greyillusion_wikipedia_960.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2016-12-21,"This year the December Solstice is today, December 21, at 10:44 UT, the first day of winter in the north and summer in the south. To celebrate, watch this amazing timelapse video tracing the Sun's apparent movement over an entire year from Hungary. During the year, a fixed video camera captured an image every minute. In total, 116,000 exposures follow the Sun's position across the field of view, starting from the 2015 June 21 solstice through the 2016 June 20 solstice. The intervening 2015 December 22 solstice is at the bottom of the frame. The timelapse sequences constructed show the Sun's movement over one day to begin with, followed by traces of the Sun's position during the days of one year, solstice to solstice. Gaps in the daily curves are due to cloud cover. The video ends with stunning animation sequences of analemmas, those figure-8 curves you get by photographing the Sun at the same time each day throughout a year, stepping across planet Earth's sky.",,video,v1,Traces of the Sun,https://www.youtube.com/embed/ZS2FvljQXsk?rel=0,"György -Bajmóczy",exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2004-12-09,"rly Tuesday morning, December 7th, June Croft thought the southeastern sky above Atmore, Alabama, USA was beautiful. Watching the Moon rise through gossamer clouds, she noted, "" ... the crescent Moon looked like it was held in the sky by a star just off its shadowed horizon."" What was that star? Bright Jupiter of course, and some watched as the Moon actually occulted or passed in front of the Solar System's reigning gas giant planet. For astronomer Jimmy Westlake in Colorado, Jupiter was already hidden at moonrise that morning, but later he was able to record this lovely image, not unlike the view that inspired Croft. Seen through gossamer clouds, Jupiter along with large Jovian satellites Ganymede and Callisto (bottom to top) has emerged from behind the crescent Moon's shadowed horizon. News: The answer to Lewin's Challenge APOD can be found here.",https://apod.nasa.gov/apod/image/0412/decMoonJup_westlake_f1.jpg,image,v1,Jupiter and the Moon's Shadowed Horizon,https://apod.nasa.gov/apod/image/0412/decMoonJup_westlake_c1.jpg," -Jimmy -Westlake -(Colorado -Mountain College) +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," + +Adam Block (Caelum +Observatory), -",exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -1997-10-14,"The month of October features a sky full of planets, including Venus as the brilliant evening star. Besides the sun and moon, Venus is the brightest object visible in Earth's sky. This month, Venus appears in early evening near the red planet Mars and Mars' red giant rival Antares above the southwestern horizon. Because it is closer to the sun than Earth, Venus never strays far from the sun in its apparent position and is seen during the year as either a bright morning or evening star. This beautiful sunset imaged from low earth orbit by the Atlantis space shuttle crew in May 1989 also reveals the planet Venus blazing above Earth's horizon. It is a fitting image for this mission and crew. It was recorded following the successful release of the robot Venus-explorer Magellan, the first planetary probe to be deployed from a space shuttle.",https://apod.nasa.gov/apod/image/9710/venus_sts30_big.jpg,image,v1,Venus On The Horizon,https://apod.nasa.gov/apod/image/9710/venus_sts30.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2023-11-27,"This eagle ray glides across a cosmic sea. Officially cataloged as SH2-63 and LBN 86, the dark nebula is composed of gas and dust that just happens to appear shaped like a common ocean fish. The interstellar dust nebula appears light brown as it blocks and reddens visible light emitted behind it. Dark nebulas glow primarily in infrared light, but also reflect visible light from surrounding stars. The dust in dark nebulas is usually sub-millimeter chunks of carbon, silicon, and oxygen, frequently coated with frozen carbon monoxide and nitrogen. Dark nebulas are also known as molecular clouds because they also contain relatively high amounts of molecular hydrogen and larger molecules. Previously unnamed, the here dubbed Eagle Ray Nebula is normally quite dim but has been imaged clearly over 20-hours through dark skies in Chile. Follow APOD on: Discord",https://apod.nasa.gov/apod/image/2311/EagleRay_Chander_3277.jpg,image,v1,LBN 86: The Eagle Ray Nebula,https://apod.nasa.gov/apod/image/2311/EagleRay_Chander_960.jpg," -Vikas Chander -",exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -1995-10-25,,https://apod.nasa.gov/apod/image/nsun_comptel.gif,image,v1,Painting with Solar Neutrons,https://apod.nasa.gov/apod/image/nsun_comptel.gif,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2000-07-24,"The Whirlpool Galaxy is a classic spiral galaxy. At only 23 million light years distant and fully 65 thousand light years across, M51, also known as NGC 5194, is one of the brightest and most picturesque galaxies on the sky. The smaller galaxy appearing here below and to the left is well behind M51, as can be inferred by the dust in a foreground spiral arm blocking light from this smaller galaxy. The Whirlpool, pictured above, is visible with binoculars in the constellation of Canes Venaciti. M51 is a spiral galaxy of type Sc and is the dominant member of a whole group of galaxies. Astronomers speculate that M51's spiral structure is primarily due to its gravitational interaction with this smaller galaxy.",https://apod.nasa.gov/apod/image/0007/m51_noao_big.jpg,image,v1,M51: The Whirlpool Galaxy,https://apod.nasa.gov/apod/image/0007/m51_noao.jpg," -Todd Boroson -(NOAO), -AURA, -NOAO, -NSF -",exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2009-09-06,"Our Earth is not at rest. The Earth moves around the Sun. The Sun orbits the center of the Milky Way Galaxy. The Milky Way Galaxy orbits in the Local Group of Galaxies. The Local Group falls toward the Virgo Cluster of Galaxies. But these speeds are less than the speed that all of these objects together move relative to the cosmic microwave background radiation (CMBR). In the above all-sky map from the COBE satellite, radiation in the Earth's direction of motion appears blueshifted and hence hotter, while radiation on the opposite side of the sky is redshifted and colder. The map indicates that the Local Group moves at about 600 kilometers per second relative to this primordial radiation. This high speed was initially unexpected and its magnitude is still unexplained. Why are we moving so fast? What is out there?",https://apod.nasa.gov/apod/image/0909/dip_cobe.gif,image,v1,CMBR Dipole: Speeding Through the Universe,https://apod.nasa.gov/apod/image/0909/dip_cobe_big.gif,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2021-11-01,"The dream was to capture both the waterfall and the Milky Way together. Difficulties included finding a good camera location, artificially illuminating the waterfall and the surrounding valley effectively, capturing the entire scene with numerous foreground and background shots, worrying that fireflies would be too distracting, keeping the camera dry, and avoiding stepping on a poisonous snake. Behold the result -- captured after midnight in mid-July and digitally stitched into a wide-angle panorama. The waterfall is the picturesque Zhulian waterfall in the Luoxiao Mountains in eastern Hunan Province, China. The central band of our Milky Way Galaxy crosses the sky and shows numerous dark dust filaments and colorful nebulas. Bright stars dot the sky -- all residing in the nearby Milky Way -- including the Summer Triangle with bright Vega visible above the Milky Way's arch. After capturing all 78 component exposures for you to enjoy, the photographer and friends enjoyed the view themselves for the rest of the night. Discovery + Outreach: Graduate student research position open for APOD",https://apod.nasa.gov/apod/image/2111/MilkyWayWaterfall_XieJie_2500.jpg,image,v1,A Waterfall and the Milky Way,https://apod.nasa.gov/apod/image/2111/MilkyWayWaterfall_XieJie_960.jpg," -Xie Jie -",exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2005-01-20,"What's happening over the water? Pictured above is one of the better images yet recorded of a waterspout, a type of tornado that occurs over water. Waterspouts are spinning columns of rising moist air that typically form over warm water. Waterspouts can be as dangerous as tornadoes and can feature wind speeds over 200 kilometers per hour. Many waterspouts form away from thunderstorms and even during relatively fair weather. Waterspouts may be relatively transparent and initially visible only by the unusual pattern they create on the water. The above image was taken in 1969 from an aircraft off the Florida Keys, a location arguably the hottest spot for waterspouts in the world with hundreds forming each year. Some people speculate that these waterspouts are responsible for many of the losses recorded in the Bermuda Triangle region of the Atlantic Ocean.",https://apod.nasa.gov/apod/image/0412/waterspout_noaa_big.jpg,image,v1,A Waterspout off the Florida Keys,https://apod.nasa.gov/apod/image/0412/waterspout_noaa.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -1999-12-16,"This false-color radio wavelength picture of an expanding stellar debris cloud is the product of one of the largest radio astronomy experiments ever. Combining the output of 20 radio telescopes scattered around planet Earth, astronomers have produced this amazingly detailed image of a supernova remnant just over 1.5 light-years across in M82, an intense star forming galaxy 12 million light-years away. The radio astronomy technique for creating the earth-sized array of telescopes is known as VLBI (very long baseline interferometry). The individual telescopes of the array are too far apart for all their signals to be combined in ""real time"", so their output was recorded on magnetic tapes which were brought to a single location and correlated. This technique has produced the highest resolution astronomical observations currently possible and allows the exploration of such distant, violent galactic environments in unprecedented detail.",https://apod.nasa.gov/apod/image/9912/m82snr_vlbi_big.gif,image,v1,Supernova Remnant In M82,https://apod.nasa.gov/apod/image/9912/m82snr_vlbi.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2002-12-04,"Gliding toward today's total eclipse of the Sun, the crescent Moon has been rising early, just before dawn. And as a prelude to its close solar alignment, the Moon also completed a lovely celestial triangle, closing with bright planets Mars and Venus on the morning of December 1. While the total solar eclipse can only be seen from a narrow corridor, skygazers around the globe could appreciate this lunar-planetary conjunction. This view is from near Nashville Tennessee, USA, and finds brilliant Venus at the lowest corner of the triangle with a much fainter Mars immediately to the right of the Moon. The Moon's sunlit crescent is overexposed, but details of the lunar night side are revealed by earthshine. Above and to the right of the trio is Spica, brightest star in the constellation Virgo.",https://apod.nasa.gov/apod/image/0212/moontrio_koehn_full.jpg,image,v1,"Moon, Mars, Venus, and Spica",https://apod.nasa.gov/apod/image/0212/moontrio_koehn.jpg," +R. Jay GaBany +(Cosmotography.com) -Larry Koehn +",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) -",exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -1997-10-30,"very day is a cloudy day on Jupiter, the Solar System's reigning gas giant. This 3-dimensional visualization presents a simplified model view from between Jovian cloud decks based on imaging and spectral data recorded by the Galileo spacecraft. The separation between the cloud layers and the height variations have been exaggerated. The upper cloud layer is haze a few tens of miles thick. Heights in the lower cloud layers have been color coded; light bluish clouds are high and thin, reddish clouds are low, and white clouds are high and thick. Streaks in the lower layer suggestively lead to a dark blue area, a relatively clear, dry region similar to the site where Galileo's atmospheric probe made the first entry into a gas giant planet's atmosphere on December 7th, 1995.",https://apod.nasa.gov/apod/image/9710/jup3dclouds_gal_big.jpg,image,v1,3-D View Of Jupiter's Clouds,https://apod.nasa.gov/apod/image/9710/jup3dclouds_gal.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2012-03-06,"Is this a painting or a photograph? In this beautiful celestial still life composed with a cosmic brush, dusty nebula NGC 2170 shines near the image center. Reflecting the light of nearby hot stars, NGC 2170 is joined by other bluish reflection nebulae, a red emission region, many dark absorption nebulae, and a backdrop of colorful stars. Like the common household items still life painters often choose for their subjects, the clouds of gas, dust, and hot stars pictured above are also commonly found in this setting - a massive, star-forming molecular cloud in the constellation of the Unicorn (Monoceros). The giant molecular cloud, Mon R2, is impressively close, estimated to be only 2,400 light-years or so away. At that distance, this canvas would be over 60 light-years across.",https://apod.nasa.gov/apod/image/1203/ngc2170_julio_1920.jpg,image,v1,NGC 2170: Celestial Still Life,https://apod.nasa.gov/apod/image/1203/ngc2170_julio_960.jpg," -Leonardo Julio & Carlos Milovic -(Astronomia Pampeana) +",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 19:36:50.197981 -2023-08-07,"The Pelican Nebula is slowly being transformed. IC 5070 (the official designation) is divided from the larger North America Nebula by a molecular cloud filled with dark dust. The Pelican, however, receives much study because it is a particularly active mix of star formation and evolving gas clouds. The featured picture was produced in three specific colors -- light emitted by sulfur, hydrogen, and oxygen -- that can help us to better understand these interactions. The light from young energetic stars is slowly transforming the cold gas to hot gas, with the advancing boundary between the two, known as an ionization front, visible in bright orange on the right. Particularly dense tentacles of cold gas remain. Millions of years from now, the Pelican nebula, bounded by dark nebula LDN 935, might no longer be known as the Pelican, as the balance and placement of stars and gas will surely leave something that appears completely different.",https://apod.nasa.gov/apod/image/2308/LDN935_Jones_1840.jpg,image,v1,"The Pelican Nebula in Gas, Dust, and Stars",https://apod.nasa.gov/apod/image/2308/LDN935_Jones_960.jpg," -Abe Jones -",exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2022-01-31,"The Great Carina Nebula is home to strange stars and iconic nebulas. Named for its home constellation, the huge star-forming region is larger and brighter than the Great Orion Nebula but less well known because it is so far south -- and because so much of humanity lives so far north. The featured image shows in great detail the northern-most part of the Carina Nebula. Visible nebulas include the semi-circular filaments surrounding the active star Wolf-Rayet 23 (WR23) on the far left. Just left of center is the Gabriela Mistral Nebula consisting of an emission nebula of glowing gas (IC 2599) surrounding the small open cluster of stars (NGC 3324). Above the image center is the larger star cluster NGC 3293, while to its right is the relatively faint emission nebula designated Loden 153. The most famous occupant of the Carina Nebula, however, is not shown. Off the image to the lower right is the bright, erratic, and doomed star star known as Eta Carinae -- a star once one of the brightest stars in the sky and now predicted to explode in a supernova sometime in the next few million years.",https://apod.nasa.gov/apod/image/2201/CarinaNorth_Colombari_3000.jpg,image,v1,Carina Nebula North,https://apod.nasa.gov/apod/image/2201/CarinaNorth_Colombari_960.jpg," -Roberto Colombari -",exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2020-11-24,"Will our Sun look like this one day? The Helix Nebula is one of brightest and closest examples of a planetary nebula, a gas cloud created at the end of the life of a Sun-like star. The outer gasses of the star expelled into space appear from our vantage point as if we are looking down a helix. The remnant central stellar core, destined to become a white dwarf star, glows in light so energetic it causes the previously expelled gas to fluoresce. The Helix Nebula, given a technical designation of NGC 7293, lies about 700 light-years away towards the constellation of the Water Bearer (Aquarius) and spans about 2.5 light-years. The featured picture was taken with the Canada-France-Hawaii Telescope (CFHT) located atop a dormant volcano in Hawaii, USA. A close-up of the inner edge of the Helix Nebula shows complex gas knots of unknown origin.",https://apod.nasa.gov/apod/image/2011/Helix2_CFHT_1917.jpg,image,v1,The Helix Nebula from CFHT,https://apod.nasa.gov/apod/image/2011/Helix2_CFHT_960.jpg," -CFHT, -Coelum, -MegaCam, -J.-C. Cuillandre -(CFHT) & -G. A. Anselmi -(Coelum) -",exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2018-07-31,"What lies beneath the layered south pole of Mars? A recent measurement with ground-penetrating radar from ESA's Mars Express satellite has detected a bright reflection layer consistent with an underground lake of salty water. The reflection comes from about 1.5 kilometers down and covers an area 20 kilometers across. Liquid water evaporates quickly from the surface of Mars, but a briny confined lake, such as implied by the radar reflection, could last much longer and be a candidate to host life such as microbes. Pictured, an infrared, green, and blue image of the south pole of Mars taken by Mars Express in 2012 shows a complex mixture of layers of dirt, frozen carbon dioxide, and frozen water.",https://apod.nasa.gov/apod/image/1807/SouthPole_MarsExpress_2310.jpg,image,v1,Layers of the South Pole of Mars,https://apod.nasa.gov/apod/image/1807/SouthPole_MarsExpress_1080.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2013-03-15,"After appearing in a popular photo opportunity with a young crescent Moon near sunset, naked-eye Comet PanSTARRS continues to rise in northern hemisphere skies. But this remarkable interplanetary perspective from March 13, finds the comet posing with our fair planet itself - as seen from the STEREO Behind spacecraft. Following in Earth's orbit, the spacecraft is nearly opposite the Sun and looks back toward the comet and Earth, with the Sun just off the left side of the frame. At the left an enormous coronal mass ejection (CME) is erupting from a solar active region. Of course, CME, comet, and planet Earth are all at different distances from the spacecraft. (The comet is closest.) The processed digital image is the difference between two consecutive frames from the spacecraft's SECCHI Heliospheric Imager, causing the strong shadowing effect for objects that move between frames. Objects that are too bright create the sharp vertical lines. The processing reveals complicated feather-like structures in Comet PanSTARRS's extensive dust tail. Growing Gallery: Comet PanSTARRS at Sunset",https://apod.nasa.gov/apod/image/1303/panstarrs_mar13_cmeV0.jpg,image,v1,"CME, Comet and Planet Earth",https://apod.nasa.gov/apod/image/1303/panstarrs_mar13_cmeV0.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2020-07-21,"Can stars, like caterpillars, transform themselves into butterflies? No, but in the case of the Butterfly Nebula -- it sure looks like it. Though its wingspan covers over 3 light-years and its estimated surface temperature exceeds 200,000 degrees, C, the dying 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 reprocessed here to show off the remarkable details of the complex planetary nebula, highlighting in particular light emitted by iron, shown in red. NGC 6302 lies about 4,000 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. Great Debates in Astronomy: 2020: How will humanity first discover extraterrestrial life?",https://apod.nasa.gov/apod/image/2007/Butterfly_HubbleSchmidt_4767.jpg,image,v1,Iron in the Butterfly Nebula,https://apod.nasa.gov/apod/image/2007/Butterfly_HubbleSchmidt_1080.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2001-08-04,"The brightest galaxy visible from our own Milky Way Galaxy is the Large Magellanic Cloud (LMC). Visible predominantly from Earth's Southern Hemisphere, the LMC is the second closest galaxy, neighbor to the Small Magellanic Cloud, and one of eleven known dwarf galaxies that orbit our Milky Way Galaxy. The LMC is an irregular galaxy composed of a bar of older red stars, clouds of younger blue stars, and a bright red star forming region visible near the top of the above image called the Tarantula Nebula. The brightest supernova of modern times, SN1987A, occurred in the LMC.",https://apod.nasa.gov/apod/image/0002/lmc_noao_big.jpg,image,v1,Neighboring Galaxy: The Large Magellanic Cloud,https://apod.nasa.gov/apod/image/0002/lmc_noao.jpg,AURA,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2020-06-04,"Sharp telescopic views of NGC 3628 show a puffy galactic disk divided by dark dust lanes. Of course, this deep portrait of the magnificent, edge-on spiral galaxy puts some astronomers in mind of its popular moniker, the Hamburger Galaxy. It also reveals a small galaxy nearby, likely a satellite of NGC 3628, and a faint but extensive tidal tail. The drawn out tail stretches for about 300,000 light-years, even beyond the right edge of the wide frame. NGC 3628 shares its neighborhood in the local universe with two other large spirals M65 and M66 in a grouping otherwise known as the Leo Triplet. Gravitational interactions with its cosmic neighbors are likely responsible for creating the tidal tail, as well as the extended flare and warp of this spiral's disk. The tantalizing island universe itself is about 100,000 light-years across and 35 million light-years away in the northern springtime constellation Leo.",https://apod.nasa.gov/apod/image/2006/N3628_StefanoCancelli_PaulMortfield.jpg,image,v1,Portrait of NGC 3628,https://apod.nasa.gov/apod/image/2006/N3628_StefanoCancelli_PaulMortfield1024.jpg,Stefano Cancelli,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2004-05-11,"M13 is one of the most prominent and best known globular clusters. Visible with binoculars in the constellation of Hercules, M13 is frequently one of the first objects found by curious sky gazers seeking celestials wonders beyond normal human vision. M13 is a colossal home to over 100,000 stars, spans over 150 light years across, lies over 20,000 light years distant, and is over 12 billion years old. At the 1974 dedication of Arecibo Observatory, a radio message about Earth was sent in the direction of M13. The reason for the low abundance of unusual blue straggler stars in M13 is currently unknown.",https://apod.nasa.gov/apod/image/0405/m13_guscott_big.jpg,image,v1,M13: The Great Globular Cluster in Hercules,https://apod.nasa.gov/apod/image/0405/m13_guscott.jpg," -Eddie Guscott -",exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2016-03-27,"How massive can a normal star be? Estimates made from distance, brightness and standard solar models had given one star in the open cluster Pismis 24 over 200 times the mass of our Sun, making it one of the most massive stars known. This star is the brightest object located just above the gas front in the featured image. Close inspection of images taken with the Hubble Space Telescope, however, have shown that Pismis 24-1 derives its brilliant luminosity not from a single star but from three at least. Component stars would still remain near 100 solar masses, making them among the more massive stars currently on record. Toward the bottom of the image, stars are still forming in the associated emission nebula NGC 6357. Appearing perhaps like a Gothic cathedral, energetic stars near the center appear to be breaking out and illuminating a spectacular cocoon.",https://apod.nasa.gov/apod/image/1603/NGC6357_hubble_3140.jpg,image,v1,NGC 6357: Cathedral to Massive Stars,https://apod.nasa.gov/apod/image/1603/NGC6357_hubble_960.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2013-09-11,"On September 6, a starry night and the Milky Way witnessed the launch of a Minotaur V rocket from NASA's Wallops Flight Facility on Wallops Island, Virginia. So did a large part of the eastern United States, as the spectacular night launch was easily visible even from light polluted urban areas. This 35 second exposure captures part of the rocket's initial launch streak and 2nd stage ignition flare along with a fiery reflection in calm waters. The stunning view faces south and west from a vantage point overlooking Sinepuxent Bay in Maryland about 20 miles north of the launch pad. Heading east over the Atlantic, the multi-stage rocket placed LADEE, the Lunar Atmosphere and Dust Environment Explorer, into a highly elliptical Earth orbit to begin its journey to the Moon.",https://apod.nasa.gov/apod/image/1309/JJB_5334_NASA-LADEE-Launch-sept2013-APOD-1000pxJB.jpg,image,v1,LADEE Launch Streak,https://apod.nasa.gov/apod/image/1309/JeffBerkes5334_NASA-LADEE-Launch-sept2013APOD900px.jpg,Jeff Berkes,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2024-06-02,"No one, presently, sees the Moon rotate like this. That's because the Earth's moon is tidally locked to the Earth, showing us only one side. Given modern digital technology, however, combined with many detailed images returned by the Lunar Reconnaissance Orbiter (LRO), a high resolution virtual Moon rotation movie has been composed. The featured time-lapse video starts with the standard Earth view of the Moon. Quickly, though, Mare Orientale, a large crater with a dark center that is difficult to see from the Earth, rotates into view just below the equator. From an entire lunar month condensed into 24 seconds, the video clearly shows that the Earth side of the Moon contains an abundance of dark lunar maria, while the lunar far side is dominated by bright lunar highlands. Currently, over 32 new missions to the Moon are under active development from multiple countries and companies, including NASA's Artemis program which aims to land people on the Moon again within the next few years.",,video,v1,Rotating Moon from LRO,https://www.youtube.com/embed/sNUNB6CMnE8?rel=0,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2003-05-13,"How big is the Sun? The Sun is not only larger than any planet, it is larger than all of the planets put together. The Sun accounts for about 99.9 percent of all the mass in its Solar System. Merely stating the Sun's diameter is about 1,400,000 kilometers does not do it justice. Last week a chance to gain visual size perspective occurred when planet Mercury made a rare crossing in front to Sun. Mercury, a planet over a third of the diameter of our Earth, is the dark dot on the upper right. In comparison to the Sun, Mercury is so small it is initially hard to spot. Also visible on the Sun are dark circular sunspots, bright plages, and dark elongated prominences -- many of which are larger than Mercury. The above contrast-enhanced picture was captured last week from France.",https://apod.nasa.gov/apod/image/0305/mercurysun_legault_big.jpg,image,v1,Mercury Transits the Sun,https://apod.nasa.gov/apod/image/0305/mercurysun_legault.jpg," -Thierry Legault -",exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2010-08-28,"This ominous, dark shape sprawling across the face of the Sun is a coronal hole -- a low density region extending above the surface where the solar magnetic field opens freely into interplanetary space. Studied extensively from space since the 1960s in ultraviolet and x-ray light, coronal holes are known to be the source of the high-speed solar wind, atoms and electrons which flow outward along the open magnetic field lines. During periods of low activity, coronal holes typically cover regions just above the Sun's poles. But this extensive coronal hole dominated the Sun's northern hemisphere earlier this week, captured here in extreme ultraviolet light by cameras onboard the Solar Dynamics Observatory. The solar wind streaming from this coronal hole triggered auroral displays on planet Earth.",https://apod.nasa.gov/apod/image/1008/CoronalHaug2010_sdo.jpg,image,v1,Hole in the Sun,https://apod.nasa.gov/apod/image/1008/CoronalHaug2010_sdo900.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2015-04-24,"Lapping at rocks along the shore of the Island of Nangan, Taiwan, planet Earth, waves are infused with a subtle blue light in this sea and night skyscape. Composed of a series of long exposures made on April 16 the image captures the faint glow from Noctiluca scintillans. Also known as sea sparkles or blue tears, the marine plankton's bioluminescence is stimulated by wave motion. City lights along the coast of mainland China shine beneath low clouds in the west but stars and the faint Milky Way still fill the night above. Over the horizon the galaxy's central bulge and dark rifts seem to echo the rocks and luminous waves.",https://apod.nasa.gov/apod/image/1504/RBA_BlueTears1600.jpg,image,v1,Blue Tears and the Milky Way,https://apod.nasa.gov/apod/image/1504/RBA_BlueTears1024.jpg,"Rogelio Bernal -Andreo",exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -1995-12-27,"In 1992 a tremendous explosion occurred in the constellation of Cygnus. Dubbed Nova Cygni 1992, this event most probably occurred in an accretion disk binary system. Astronomers hypothesize that this system's white dwarf had so much gas dumped onto it's surface that conditions became ripe for nuclear fusion. The resulting thermonuclear detonation blasted much of the surrounding gas into an expanding shell. The Hubble Space Telescope photographed this expanding shell in 1994. Nova Cygni 1992 was the brightest nova in recent history - at its brightest it could be seen without a telescope. It was observed in every part of the electromagnetic spectrum.",https://apod.nasa.gov/apod/image/novaCygni_hst.gif,image,v1,Nova Cygni 1992,https://apod.nasa.gov/apod/image/novaCygni_hst.gif,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2007-04-03,"Why would clouds form a hexagon on Saturn? Nobody is yet sure. Originally discovered during the Voyager flybys of Saturn in the 1980s, nobody has ever seen anything like it anywhere else in the Solar System. If Saturn's South Pole wasn't strange enough with its rotating vortex, Saturn's North Pole might now be considered even stranger. The bizarre cloud pattern is shown above in a recent infrared image taken by the Saturn-orbiting Cassini spacecraft. The images show the stability of the hexagon even 20 years after Voyager. Movies of Saturn's North Pole show the cloud structure maintaining its hexagonal structure while rotating. Unlike individual clouds appearing like a hexagon on Earth, the Saturn cloud pattern appears to have six well defined sides of nearly equal length. Four Earths could fit inside the hexagon. Although full explanations are not yet available, planetary scientists are sure to continue to study this most unusual cloud formation for quite some time.",https://apod.nasa.gov/apod/image/0704/hexagon_cassini_big.jpg,image,v1,A Mysterious Hexagonal Cloud System on Saturn,https://apod.nasa.gov/apod/image/0704/hexagon_cassini.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2013-11-14,"gmatic spiral galaxy NGC 1097 shines in southern skies, about 45 million light-years away in the chemical constellation Fornax. Its blue spiral arms are mottled with pinkish star forming regions in this colorful galaxy portrait. They seem to have wrapped around a small companion galaxy below and left of center, about 40,000 light-years from the spiral's luminous core. That's not NGC 1097's most peculiar feature, though. The very deep exposure hints of faint, mysterious jets, most easily seen to extend well beyond the bluish arms toward the lower right. In fact, four faint jets are ultimately recognized in optical images of NGC 1097. The jets trace an X centered on the galaxy's nucleus, but probably don't originate there. Instead, they could be fossil star streams, trails left over from the capture and disruption of a much smaller galaxy in the large spiral's ancient past. A Seyfert galaxy, NGC 1097's nucleus also harbors a supermassive black hole.",https://apod.nasa.gov/apod/image/1311/NGC1097HaLRGBpugh.jpg,image,v1,The Jets of NGC 1097,https://apod.nasa.gov/apod/image/1311/NGC1097HaLRGBpugh950.jpg,Martin Pugh,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2005-02-07,"What do you get when you combine one of the world's most powerful telescopes with a powerful laser? An artificial star. Monitoring fluctuations in brightness of a genuine bright star can indicate how the Earth's atmosphere is changing, but many times no bright star exists in the direction where atmospheric information is needed. Therefore, astronomers have developed the ability to create an artificial star where they need it -- with a laser. Subsequent observations of the artificial laser guide star can reveal information so detailed about the blurring effects of the Earth's atmosphere that much of this blurring can be removed by rapidly flexing the mirror. Such adaptive optic techniques allow high-resolution ground-based observations of real stars, planets, nebulae, and the early universe. Above, a laser beam shoots out of the Keck II 10-meter telescope on Mauna Kea in Hawaii in 2002, creating an artificial star.",https://apod.nasa.gov/apod/image/0502/laser_keck_big.jpg,image,v1,A Telescope Laser Creates an Artificial Star,https://apod.nasa.gov/apod/image/0502/laser_keck.jpg,"Adam Contos -(Ball Aerospace) -",exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2020-10-27,"What would an erupting volcano on Venus look like? Evidence of currently active volcanoes on Venus was announced earlier this year with the unexplained warmth of regions thought to contain only ancient volcanoes. Although large scale images of Venus have been taken with radar, thick sulfuric acid clouds would inhibit the taking of optical light vistas. Nevertheless, an artist's reconstruction of a Venusian volcano erupting is featured. Volcanoes could play an important role in a life cycle on Venus as they could push chemical foods into the cooler upper atmosphere where hungry microbes might float. Pictured, the plume from an erupting volcano billows upwards, while a vast lava field covers part of the hot and cracked surface of Earth's overheated twin. The possibility of airborne microbial Venusians is certainly exciting, but currently controversial. An APOD Described on TikTok: By astrokirsten",https://apod.nasa.gov/apod/image/2010/VenusVolcano_NasaRubin_1600.jpg,image,v1,Venusian Volcano Imagined,https://apod.nasa.gov/apod/image/2010/VenusVolcano_NasaRubin_1080.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2005-09-12,"Is this one galaxy or two? The jumble of stars, gas, and dust that is NGC 520 is now thought to incorporate the remains of two separate galaxies. A combination of observations and simulations indicate the NGC 520 is actually the collision of two disk galaxies. Interesting features of NGC 520 include an unfamiliar looking tail of stars at the image bottom and a perhaps more familiar looking band of dust running diagonally across the image center. A similar looking collision might be expected were our disk Milky Way Galaxy to collide with our large galactic neighbor Andromeda (M31). The collision that defines NGC 520 started about 300 million years ago and continues today. Although the speeds of stars are fast, the distances are so vast that the interacting pair will surely not change its shape noticeably during our lifetimes. NGC 520, at visual magnitude 12, has been noted to be one of the brightest interacting galaxies on the sky, after interacting pairs of galaxies known as the Antennae. NGC 520 was imaged above in spectacular fashion by the Gemini Observatory in Hawaii, USA. Also known as Arp 157, NGC 520 lies about 100 million light years distant, spans about 100 thousand light years, and can be seen with a small telescope toward the constellation of the Fish (Pisces).",https://apod.nasa.gov/apod/image/0509/ngc520_gemini_big.jpg,image,v1,The Colliding Galaxies of NGC 520,https://apod.nasa.gov/apod/image/0509/ngc520_gemini.jpg,Gemini Obs.,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2010-07-28,"Unspeakable beauty and unimaginable bedlam can be found together in the Trifid Nebula. Also known as M20, this photogenic nebula is visible with good binoculars towards the constellation of Sagittarius. The energetic processes of star formation create not only the colors but the chaos. The red-glowing gas results from high-energy starlight striking interstellar hydrogen gas. The dark dust filaments that lace M20 were created in the atmospheres of cool giant stars and in the debris from supernovae explosions. Which bright young stars light up the blue reflection nebula is still being investigated. The light from M20 we see today left perhaps 3,000 years ago, although the exact distance remains unknown. Light takes about 50 years to cross M20.",https://apod.nasa.gov/apod/image/1007/m20_gendler_big.jpg,image,v1,The Trifid Nebula is Stars and Dust,https://apod.nasa.gov/apod/image/1007/m20_gendler.jpg,Robert Gendler,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2002-02-23,"Fifteen years ago today, the brightest supernova of modern times was sighted. Over time, astronomers have watched and waited for the expanding debris from this tremendous stellar explosion to crash into previously expelled material. A clear result of such a collision is demonstrated above in two frames recorded by the Hubble Space Telescope in 1994 (left) and 1997(right). While the central concentration of stellar debris has clearly evolved over this period, the yellow spot on the ring in the righthand picture announces the collision of an outward moving blast wave with the pre-existing, light-year wide ring. The collision is occurring at speeds near 60 million kilometers per hour and shock-heats the ring material causing it to glow. Astronomers are hopeful that such collisions will illuminate the interesting past of SN 1987A, and perhaps provide more clues about the origin of the mysterious rings.",https://apod.nasa.gov/apod/image/0202/sn87aknot_hst_big.jpg,image,v1,Shocked by Supernova 1987A,https://apod.nasa.gov/apod/image/0202/sn87aknot_hst.jpg,,exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -2007-02-26,"What's that cloud drifting in space? It's not an astronomical nebula -- those appear to stay put. Atmospheric clouds don't look like this. The answer to last week's sky mystery turned out to be orbiting and expanding debris from the upper stage of a failed Russian rocket that exploded unexpectedly. The cloud became visible to unaided southern hemisphere observers, and its cause was initially unknown. The above time lapse movie shows the cloud drifting as seen from Australia. Streaks in and near the cloud are likely large pieces of debris. The debris cloud is more than an astronomical curiosity -- particles from this cloud and others could become projectiles damaging existing satellites. As the cloud disperses, many particles will fall to Earth, but many more may help make low Earth orbit an increasingly hostile environment.",https://apod.nasa.gov/apod/image/0702/debrismovie_mcnaught_big.gif,image,v1,A Rocket Debris Cloud Drifts,https://apod.nasa.gov/apod/image/0702/debrismovie_mcnaught.jpg," -Robert H. McNaught -",exoplanet,,,,,,,,,,,,,,NASA,2024-12-20 19:36:50.197981 -,,,,,,,,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': 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'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 19:36:50.197981 -,,,,,,,,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 19:36:50.197981 +",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': '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', 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{'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', 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