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APOD https://apod.nasa.gov/Astronomy Picture of the Day Sun, 17 Nov 2024 05:05:26 GMT https://validator.w3.org/feed/docs/rss2.html https://github.com/etabits/apodrss en APOD https://apod.nasa.gov/favicon.ico https://apod.nasa.gov/APOD.nasa.gov <![CDATA[LDN 1471: A Windblown Star Cavity]]> https://apod.nasa.gov/apod/ap241117.htmlhttps://apod.nasa.gov/apod/ap241117.html Hubble NASA ESA License Judy Schmidt Robert Nemiroff (MTU) Jerry Bonnell (UMCP) Sun, 17 Nov 2024 12:00:00 GMT
Explanation: What is the cause of this unusual parabolic structure? This illuminated cavity, known as LDN 1471, was created by a newly forming star, seen as the bright source at the peak of the parabola. This protostaris experiencing a stellar outflow which is then interacting with the surrounding material in the Perseus Molecular Cloud, causing it to brighten. We see only one side of the cavity -- the other side is hidden by dark dust. The parabolic shape is caused by the widening of the stellar-wind blown cavity over time. Two additional structures can also be seen either side of the protostar; these are known as Herbig-Haro objects, again caused by the interaction of the outflow with the surrounding material. What causes the striations on the cavity walls, though, remains unknown. The featured image was taken by NASA and ESA’s Hubble Space Telescope after an original detection by the Spitzer Space Telescope.]]> <![CDATA[Pluto at Night]]> https://apod.nasa.gov/apod/ap241116.htmlhttps://apod.nasa.gov/apod/ap241116.html NASA Johns Hopkins Univ./APL Southwest Research Institute Robert Nemiroff (MTU) Jerry Bonnell (UMCP) Sat, 16 Nov 2024 12:00:00 GMT
Explanation: The night side of Pluto spansthis shadowy scene. In the stunning spacebased perspective the Sun is 4.9 billion kilometers (almost 4.5 light-hours) behind the dim and distant world. It was captured by far flungNew Horizons in July of 2015when the spacecraft was at a range of some 21,000 kilometers from Pluto, about 19 minutes after its closest approach. A denizenof the Kuiper Beltin dramatic silhouette, the image also reveals Pluto's tenuous, surprisinglycomplex layersof hazy atmosphere. Near the top of the frame the crescent twilight landscape includes southern areas of nitrogen ice plains now formally known asSputnik Planitiaandrugged mountainsof water-ice in the Norgay Montes.]]> <![CDATA[Apollo 12 and Surveyor 3]]> https://apod.nasa.gov/apod/ap241115.htmlhttps://apod.nasa.gov/apod/ap241115.html NASA Apollo 12 Alan Bean Kevin Frank Robert Nemiroff (MTU) Jerry Bonnell (UMCP) Fri, 15 Nov 2024 12:00:00 GMT
Explanation: Put on yourred/blue glassesand gaze across the westernOcean of Stormson the surface of the Moon.The 3D anaglyph features Apollo 12 astronaut Pete Conradvisiting the Surveyor 3 spacecraft in November of 1969.Surveyor 3 had landed at the site on the inside slope of a small crater about 2 1/2 years earlier in April of 1967. Visible on the horizon beyond the far crater wall, Apollo 12'sLunar Module Intrepidtouched down less than 200 meters (650 feet) away, easy moonwalking distance from the robotic Surveyor spacecraft. This stereo image was carefully created from two separate pictures(AS12-48-7133, AS12-48-7134)captured on thelunar surface. They depict the scene from only slightly different viewpoints, approximating the separation between human eyes.]]> <![CDATA[IC 348 and Barnard 3]]> https://apod.nasa.gov/apod/ap241114.htmlhttps://apod.nasa.gov/apod/ap241114.html Ashraf Abu Sara Robert Nemiroff (MTU) Jerry Bonnell (UMCP) Thu, 14 Nov 2024 12:00:00 GMT
Explanation: A great nebulous regionnear bright star omicron Persei offers this study in cosmic contrasts. Captured inthe telescopic frameis a colorful complex of dust, gas, and stars spanning about 3 degrees on the sky along the edge of thePerseus molecular cloud, some 1000 light-years away. Surrounded by a bluish halo of dust-reflected starlight, omicron Persei itself is just left of center. Immediately below it lies the intriguing young star cluster IC 348recently explored at infrared wavelengths by the James Webb Space Telescope. In silhouette against the diffuse reddish glow ofhydrogen gas, dark and obscuring interstellar dust cloud Barnard 3 is at upper right. Of course, the cosmic dust also tends to hide newly formed stars and young stellar objects or protostars from prying optical telescopes. At the Perseus molecular cloud'sestimated distance, this field of view would span about 50 light-years.]]> <![CDATA[Barred Spiral Galaxy NGC 1365 from Webb]]> https://apod.nasa.gov/apod/ap241113.htmlhttps://apod.nasa.gov/apod/ap241113.html NASA ESA CSA NOIRLab STScI Robert Nemiroff (MTU) Jerry Bonnell (UMCP) Wed, 13 Nov 2024 12:00:00 GMT
Explanation: A mere56 million light-years distant toward the southern constellation Fornax,NGC 1365 is an enormousbarred spiral galaxy about 200,000 light-years in diameter. That's twice the size of our own barred spiral Milky Way.This sharp imagefrom theJames Webb Space Telescope's Mid-Infrared Instrument (MIRI)reveals stunning detailsof this magnificent spiralin infrared light. Webb'sfield of viewstretches about 60,000 light-years across NGC 1365, exploring the galaxy's core and bright newborn star clusters. The intricate network of dusty filaments and bubbles is created by young stars along spiral arms winding from the galaxy's central bar.Astronomers suspectthe gravity field of NGC 1365's bar plays a crucial role in the galaxy's evolution, funneling gas and dust into astar-forming maelstromand ultimately feeding material into the active galaxy's central,supermassive black hole.]]> <![CDATA[NGC 6888: The Crescent Nebula]]> https://apod.nasa.gov/apod/ap241112.htmlhttps://apod.nasa.gov/apod/ap241112.html Team ARO Robert Nemiroff (MTU) Jerry Bonnell (UMCP) Tue, 12 Nov 2024 12:00:00 GMT
Explanation: How was the Crescent Nebula created? Looking like an emerging space cocoon, the Crescent Nebula, visible in the center of the featured image, was created by the brightest star in its center. A leading progenitor hypothesis has the Crescent Nebulabeginning to form about 250,000 years ago. At that time, the massive central star had evolved to become a Wolf-Rayet star (WR 136), shedding its outer envelope in a strong stellar wind, ejecting the equivalent of our Sun's mass every 10,000 years. This wind impacted surrounding gas left over from a previous phase, compacting it into a series of complex shells, and lighting it up. The Crescent Nebula, also known as NGC 6888, lies about 4,700 light-years away in the constellation of Cygnus. Star WR 136 will probably undergo a supernovaexplosion sometime in the next million years.]]> <![CDATA[The Unusual Tails of Comet Tsuchinshan-Atlas]]> https://apod.nasa.gov/apod/ap241111.htmlhttps://apod.nasa.gov/apod/ap241111.html Bray Falls Robert Nemiroff (MTU) Jerry Bonnell (UMCP) Mon, 11 Nov 2024 12:00:00 GMT
Explanation: What created an unusual dark streak in Comet Tsuchinshan-Atlas's tail? Some images of the bright comet during mid-October not only caught its impressively long tail and its thin anti-tail, but a rather unexpected feature: a dark streak in the long tail. The reason for the dark streak is currently unclear and a topic of some debate. Possible reasons include a plume of dark dust, different parts of the bright tailbeing unusually superposed, and a shadow of a dense part of the coma on smaller dust particles. The streak is visible in the featured image taken on October 14 from Texas, USA. To help future analyses, if you have taken a good image of the comet that clearly shows this dark streak, please send it in to APOD. Comet Tsuchinshan–ATLAShas now faded considerably and is returning to the outer Solar System.]]> <![CDATA[Valles Marineris: The Grand Canyon of Mars]]> https://apod.nasa.gov/apod/ap241110.htmlhttps://apod.nasa.gov/apod/ap241110.html NASA USGS Viking Project Robert Nemiroff (MTU) Jerry Bonnell (UMCP) Sun, 10 Nov 2024 12:00:00 GMT
Explanation: The largest canyon in the Solar Systemcuts a wide swath across the face of Mars. Named Valles Marineris, the grand valley extends over 3,000 kilometers long, spans as much as 600 kilometers across, and delves as much as 8 kilometers deep. By comparison, the Earth's Grand Canyonin Arizona, USA is 800 kilometers long, 30 kilometers across, and 1.8 kilometers deep. The origin of the Valles Marineris remains unknown, although a leading hypothesis holds that it started as a crack billions of years ago as the planet cooled. Several geologic processes have been identified in the canyon. The featured mosaic was created from over 100 images of Mars taken by Viking Orbiters in the 1970s.]]> <![CDATA[Neptune at Night]]> https://apod.nasa.gov/apod/ap241109.htmlhttps://apod.nasa.gov/apod/ap241109.html Voyager NASA Robert Nemiroff (MTU) Jerry Bonnell (UMCP) Sat, 09 Nov 2024 12:00:00 GMT
Explanation: Ice giant Neptuneis faint in Earth's night sky. Some 30 times farther from the Sun than our fair planet, telescopes are needed tocatch a glimpseof the dim and distant world. This dramatic view ofNeptune's nightjust isn't possible for telescopes in the vicinity of planet Earth though. Peering out from the inner Solar System they can only bringNeptune's day side into view. In fact this night side image with Neptune's slender crescent next to the crescent of its large moon Triton was captured by Voyager 2. Launched from planet Earth in 1977 theVoyager 2 spacecraftmade a close fly by of the Solar System's outermost planet in 1989, looking back on Neptune at night as the robotic spacecraft continued itsvoyage to interstellar space.]]> <![CDATA[Helping Hand in Cassiopeia]]> https://apod.nasa.gov/apod/ap241108.htmlhttps://apod.nasa.gov/apod/ap241108.html Francesco Radici Robert Nemiroff (MTU) Jerry Bonnell (UMCP) Fri, 08 Nov 2024 12:00:00 GMT
Explanation: Drifting nearthe plane of our Milky Way galaxy these dusty molecular clouds seem to extend a helping hand on a cosmic scale. Part of alocal complexof star-forming interstellar clouds they include LDN 1358, 1357, and 1355 from American astronomer Beverly Lynds' 1962Catalog of Dark Nebulae. Presenting achallenging targetfor astro-imagers, the obscuring dark nebulae are nearly 3,000 light-years away, toward rich starfields in the northern constellationCassiopeia. At that distance, this deep, telescopic field of view would span about 80 light-years.]]> <![CDATA[Shell Galaxies in Pisces]]> https://apod.nasa.gov/apod/ap241107.htmlhttps://apod.nasa.gov/apod/ap241107.html George Williams Robert Nemiroff (MTU) Jerry Bonnell (UMCP) Thu, 07 Nov 2024 12:00:00 GMT
Explanation: This spectacularintergalactic skyscape features Arp 227, a curious system of galaxies from the 1966Atlas of Peculiar Galaxies. Some 100 million light-years distant within the boundaries of the constellation Pisces, Arp 227 consists of the two galaxies prominent above and left of center, theshell galaxy NGC 474and its blue, spiral-armed neighbor NGC 470. The readily apparent shells and star streams ofNGC 474 are likely tidal featuresoriginating from the accretion of another smaller galaxy during close gravitational encounters that began over a billion years ago. The large galaxy on the bottom righthand side of the deep image, NGC 467, appears to be surrounded by faint shells and streams too, evidence of anothermerging galaxy system. Intriguing background galaxies are scattered around the field that also includes spiky foreground stars. Of course, those stars lie well within our ownMilky Way Galaxy. The telescopic field of view spans 25 arc minutes or just under 1/2 degreeon the sky.]]> <![CDATA[Comet Tsuchinshan-Atlas over the Dolomites]]> https://apod.nasa.gov/apod/ap241106.htmlhttps://apod.nasa.gov/apod/ap241106.html Alessandra Masi Robert Nemiroff (MTU) Jerry Bonnell (UMCP) Wed, 06 Nov 2024 12:00:00 GMT
Explanation: Comet Tsuchinshan-Atlas is now headed back to the outer Solar System. The massive dusty snowball put on quite a show during its trip near the Sun, resulting in many impressive pictures from planet Earth during October. The featured image was taken in mid-October and shows a defining visual feature of the comet -- its impressive anti-tail. The image captures Comet C/2023 A3 (Tsuchinshan–ATLAS) with impressively long dust and ion tails pointing up and away from the Sun, while the strong anti-tail -- composed of more massive dust particles -- trails the comet and points down and (nearly) toward the recently-set Sun. In the foreground is village of Tai di Cadore, Italy, with the tremendous Dolomite Mountains in the background. Another comet, C/2024 S1 (ATLAS), once a candidate to rival Comet Tsuchinshan-Atlas in brightness, broke up last week during its close approach to our Sun.]]> <![CDATA[Milky Way over Easter Island]]> https://apod.nasa.gov/apod/ap241105.htmlhttps://apod.nasa.gov/apod/ap241105.html Josh Dury Robert Nemiroff (MTU) Jerry Bonnell (UMCP) Tue, 05 Nov 2024 12:00:00 GMT
Explanation: Why were the statues on Easter Island built? No one is sure. What is sure is that over 900 large stone statues called moais exist there. The Rapa Nui (Easter Island) moais stand, on average, over twice as tall as a person and have over 200 times as much mass. It is thought that the unusual statues were created about 600 years ago in the images of local leaders of a vibrant and ancient civilization. Rapa Nui has been declared by UNESCO to a World Heritage Site.Pictured here, some of the stone giants were imaged last month under the central band of our Milky Way galaxy. Previously unknown moais are still being discovered.]]> <![CDATA[M42: The Great Nebula in Orion]]> https://apod.nasa.gov/apod/ap241104.htmlhttps://apod.nasa.gov/apod/ap241104.html Fényes Lóránd Robert Nemiroff (MTU) Jerry Bonnell (UMCP) Mon, 04 Nov 2024 12:00:00 GMT
Explanation: The Great Nebula in Orion, an immense, nearby starbirth region, is probably the most famous of all astronomical nebulas. Here, glowing gassurrounds hot young stars at the edge of an immense interstellar molecular cloud only 1500 light-years away. In the featured deep image in assigned colorshighlighted by emission in oxygen and hydrogen, wisps and sheets of dustand gas are particularly evident. The Great Nebula in Orioncan be found with the unaided eye near the easily identifiablebelt of three stars in the popular constellation Orion. In addition to housing a bright open cluster of stars known as the Trapezium, the Orion Nebula contains many stellar nurseries. These nurseries contain much hydrogen gas, hot young stars, proplyds, and stellar jetsspewing material at high speeds. Also known as M42, the Orion Nebula spans about 40 light years and is located in the same spiral arm of our Galaxy as the Sun.]]> <![CDATA[Jupiter Abyss]]> https://apod.nasa.gov/apod/ap241103.htmlhttps://apod.nasa.gov/apod/ap241103.html NASA Juno SwRI MSSS License Gerald Eichstädt Sean Doran Robert Nemiroff (MTU) Jerry Bonnell (UMCP) Sun, 03 Nov 2024 12:00:00 GMT
Explanation: What's that black spot on Jupiter? No one is sure. During one pass of NASA's Juno over Jupiter, the robotic spacecraft imaged an usually dark cloud feature informally dubbed the Abyss. Surrounding cloud patterns show the Abyss to be at the center of a vortex. Since dark features on Jupiter's atmosphere tend to run deeper than light features, the Abyss may really be the deep hole that it appears -- but without more evidence that remains conjecture. The Abyss is surrounded by a complex of meandering clouds and other swirling storm systems, some of which are topped by light colored, high-altitude clouds. The featured image was captured in 2019 while Juno passedonly about 15,000 kilometers above Jupiter's cloud tops. The next close pass of Juno near Jupiter will be in about three weeks.]]> <![CDATA[Saturn at Night]]> https://apod.nasa.gov/apod/ap241102.htmlhttps://apod.nasa.gov/apod/ap241102.html NASA JPL-Caltech Space Science Institute Mindaugas Macijauskas Robert Nemiroff (MTU) Jerry Bonnell (UMCP) Sat, 02 Nov 2024 11:00:00 GMT
Explanation: Saturn is brightin Earth's night skies. Telescopic views of the outer gas giant planet 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 in the vicinity of planet Earth. Peering out from the inner Solar System they can only bringSaturn's day side 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 mosaicis composed of frames recordedby Cassini'swide-angle camera only two days before itsgrand final plunge. Saturn's night will not be seen again untilanother spaceshipfrom Earth calls.]]> <![CDATA[Spiral Galaxy NGC 6744]]> https://apod.nasa.gov/apod/ap241101.htmlhttps://apod.nasa.gov/apod/ap241101.html John Hayes Robert Nemiroff (MTU) Jerry Bonnell (UMCP) Fri, 01 Nov 2024 11:00:00 GMT
Explanation: Big,beautiful spiral galaxy NGC 6744is nearly 175,000 light-years across, larger thanour own Milky Way. It lies some 30 million light-years distant in the southern constellation Pavo but appears as only a faint smudge in the eyepiece of a small telescope. We see the disk of the nearby island universe tilted towards our line of sight in this remarkably deep and detailed galaxy portrait, a telescopic image that spans an area about the angular size of a full moon. In it, the giant galaxy'selongated yellowish coreis dominated by the light from old, cool stars. Beyond the core, grand spiral arms are filled with young blue star clusters and speckled with pinkish star forming regions. An extended arm sweeps past smaller satellite galaxy NGC 6744A at the upper left. NGC 6744's galactic companion is reminiscent of the Milky Way's satellite galaxy the Large Magellanic Cloud.]]> <![CDATA[Rigel and the Witch Head Nebula]]> https://apod.nasa.gov/apod/ap241031.htmlhttps://apod.nasa.gov/apod/ap241031.html Simone Curzi Robert Nemiroff (MTU) Jerry Bonnell (UMCP) Thu, 31 Oct 2024 11:00:00 GMT
Explanation: By starlight, this eerie visage shines in the dark with a crooked profile evoking its popular name, theWitch Head Nebula. In fact, this entrancingtelescopic portraitgives the impression that a witch has fixed her gaze on Orion's bright supergiantstar Rigel. More formally known asIC 2118, the Witch Head Nebula spans about 50 light-years and is composed of interstellar dust grains reflecting Rigel's starlight. The color of the Witch Head Nebula is caused not only by Rigel's intense blue light, but because thedust grains scatter blue light more efficiently than red. The samephysical processcausesEarth's daytime skyto appear blue, although the scatterers in Earth's atmosphere are molecules of nitrogen and oxygen. Rigel and this dusty cosmic crone are about 800 light-years away. You may still see a few witches in your neighborhood tonight though, so have a safe andHappy Halloween!]]> <![CDATA[NGC 7635: The Bubble Nebula]]> https://apod.nasa.gov/apod/ap241030.htmlhttps://apod.nasa.gov/apod/ap241030.html Chad Leader Robert Nemiroff (MTU) Jerry Bonnell (UMCP) Wed, 30 Oct 2024 11:00:00 GMT
Explanation: What created this huge space bubble? Blown by the wind from a star, thistantalizing, head-like apparition is cataloged as NGC 7635, but known simply as the Bubble Nebula. The featured striking view utilizes a long exposure to reveal the intricate details ofthis cosmic bubble and its environment. Although it looks delicate, the 10 light-yeardiameter bubble offers evidence ofviolent processes at work. Seen here above and right of the Bubble's center, a bright hot star is embedded in the nebula's reflecting dust. A fierce stellar windand intense radiation from the star, which likely has a mass 10 to 20 times that of the Sun, has blasted out thestructure of glowing gasagainst denser material in a surrounding molecular cloud. The intriguing Bubble Nebula lies a mere 11,000 light-years away toward the boastful constellation Cassiopeia.]]> <![CDATA[NGC 602: Stars Versus Pillars from Webb]]> https://apod.nasa.gov/apod/ap241029.htmlhttps://apod.nasa.gov/apod/ap241029.html ESA Webb NASA CSA P. Zeidler E. Sabbi A. Nota M. Zamani ESA/Webb Robert Nemiroff (MTU) Jerry Bonnell (UMCP) Tue, 29 Oct 2024 11:00:00 GMT
Explanation: The stars are destroying the pillars. More specifically, some of the newly formed stars in the image center are emitting light so energetic that is evaporatingthe gas and dust in the surrounding pillars. Simultaneously, the pillars themselves are still trying to form new stars. The whole setting is the star cluster NGC 602, and this new vista was taken by the Webb Space Telescope in multiple infrared colors. In comparison, a roll-over image shows the same star cluster in visible light, taken previously by the Hubble Space Telescope. NGC 602 is located near the perimeter of the Small Magellanic Cloud (SMC), a small satellite galaxy of our Milky Way galaxy. At the estimated distance of the SMC, the featured picture spans about 200 light-years. A tantalizing assortment of background galaxies are also visible -- mostly around the edges -- that are at least hundreds of millions of light-years beyond.]]> <![CDATA[STEVE: A Glowing River over France]]> https://apod.nasa.gov/apod/ap241028.htmlhttps://apod.nasa.gov/apod/ap241028.html Louis LEROUX-GÉRÉ Robert Nemiroff (MTU) Jerry Bonnell (UMCP) Mon, 28 Oct 2024 11:00:00 GMT
Explanation: Sometimes a river of hot gas flows over your head. In this case the river created a Strong Thermal Emission Velocity Enhancement (STEVE) that glowed bright red, white, and pink. Details of how STEVEs work remain a topic of research, but recent evidence holds that their glow results from a fast-moving river of hot ionsflowing over a hundred kilometers up in the Earth's atmosphere: the ionosphere. The more expansive dull red glow might be related to the flowing STEVE, but alternatively might be a Stable Auroral Red (SAR) arc, a more general heat-related glow. The featured picture, taken earlier this month in Côte d'Opale, France, is a wide-angle digital composite made as the STEVE arc formed nearly overhead. Although the apparition lasted only a few minutes, this was long enough for the quick-thinking astrophotographer to get in the picture -- can you find him?]]> <![CDATA[LDN 43: The Cosmic Bat Nebula]]> https://apod.nasa.gov/apod/ap241027.htmlhttps://apod.nasa.gov/apod/ap241027.html Mark Hanson Mike Selby Michelle Thaller NASA GSFC Robert Nemiroff (MTU) Jerry Bonnell (UMCP) Sun, 27 Oct 2024 11:00:00 GMT
Explanation: What is the most spook-tacular nebula in the galaxy? One contender is LDN 43, which bears an astonishing resemblance to a vast cosmic bat flying amongst the stars on a dark Halloween night. Located about 1400 light yearsaway in the constellation Ophiuchus, this molecular cloud is dense enough to block lightnot only from background stars, but from wisps of gas lit up by the nearby reflection nebula LBN 7. Far from being a harbinger of death, this 12-light year-long filament of gas and dust is actually a stellar nursery. Glowing with eerie light, the bat is lit up from inside by dense gaseous knots that have just formed young stars.]]> <![CDATA[Phantoms in Cassiopeia]]> https://apod.nasa.gov/apod/ap241026.htmlhttps://apod.nasa.gov/apod/ap241026.html Christophe Vergnes Robert Nemiroff (MTU) Jerry Bonnell (UMCP) Sat, 26 Oct 2024 11:00:00 GMT
Explanation: These brightly outlined flowing shapes look ghostly on a cosmic scale.A telescopic viewtoward the constellationCassiopeia, the colorful skyscape features the swept-back, comet-shaped clouds IC 59 (left) and IC 63. About 600 light-years distant,the cloudsaren't actually ghosts. They are slowly disappearing though, under the influence ofenergetic radiationfrom hot, luminous star gamma Cas.Gamma Cas is physically located only 3 to 4 light-years from the nebulae and lies just above the right edge of the frame. Slightly closer to gamma Cas, IC 63 is dominated byred H-alpha light emitted as hydrogen atoms ionized by the hot star's ultraviolet radiation recombine with electrons. Farther from the star, IC 59 shows less H-alpha emission but more of the characteristic blue tint of dustreflected star light. The field of view spans over 1 degree or 10 light-years at the estimated distance ofthe interstellar apparitions.]]> <![CDATA[Globular Star Cluster NGC 6752]]> https://apod.nasa.gov/apod/ap241025.htmlhttps://apod.nasa.gov/apod/ap241025.html Massimo Di Fusco Aygen Erkaslan Robert Nemiroff (MTU) Jerry Bonnell (UMCP) Fri, 25 Oct 2024 11:00:00 GMT
Explanation: Some 13,000 light-years away toward the southern constellation Pavo, the globular star cluster NGC 6752 roams the halo of our Milky Way galaxy. Over 10 billion years old,NGC 6752follows clustersOmega Centauri,47 Tucanae, andMessier 22as the fourth brightest globular in planet Earth's night sky. It holds over 100 thousandstars in a sphereabout 100 light-years in diameter. Telescopicexplorationsof NGC 6752 have found that a remarkable fraction of the stars near the cluster's core are multiple star systems. They also reveal the presence of blue straggle stars, stars which appear to be too young and massive to exist in a cluster whose stars are all expected to be at least twice as old as the Sun. The blue stragglers arethought to beformed by star mergers and collisions in the dense stellar environment at the cluster'score. Thissharp color compositealso features the cluster's ancient red giant stars in yellowish hues. (Note: The bright, spiky blue star about 8 o'clock from the cluster center is a foreground star along the line-of-sight to NGC 6752)]]> <![CDATA[NGC 7293: The Helix Nebula]]> https://apod.nasa.gov/apod/ap241024.htmlhttps://apod.nasa.gov/apod/ap241024.html Patrick Winkler Robert Nemiroff (MTU) Jerry Bonnell (UMCP) Thu, 24 Oct 2024 11:00:00 GMT
Explanation: A mere seven hundred light years from Earth toward the constellationAquarius, a star is dying. The once sun-like star's last few thousand years have produced theHelix Nebula. Also known as NGC 7293, the cosmic Helix is a well studied and nearby example of aPlanetary Nebula, typical of this final phase of stellar evolution. Combining narrow band data from emission lines of hydrogen atoms in red and oxygen atoms in blue-green hues, this deep image shows tantalizingdetailsof the Helix, including its brightinner regionabout 3 light-years across. The white dot at the Helix's center is this Planetary Nebula's hot, dyingcentral star. A simple looking nebula at first glance, the Helix is now understood to have a surprisinglycomplex geometry.]]> <![CDATA[M16: Pillars of Star Creation]]> https://apod.nasa.gov/apod/ap241022.htmlhttps://apod.nasa.gov/apod/ap241022.html NASA ESA CSA STScI Diego Pisano Robert Nemiroff (MTU) Jerry Bonnell (UMCP) Tue, 22 Oct 2024 11:00:00 GMT
Explanation: These dark pillars may look destructive, but they are creating stars. This pillar-capturing picture of the Eagle Nebula combines visible light exposures taken with the Hubble Space Telescope with infrared images taken with the James Webb Space Telescope to highlight evaporating gaseous globules (EGGs) emerging from pillars of molecular hydrogen gas and dust. The giant pillars are light years in length and are so dense that interior gas contracts gravitationally to form stars. At each pillar's end, the intense radiation of bright young stars causes low density material to boil away, leaving stellar nurseries of dense EGGs exposed. The Eagle Nebula, associated with the open star cluster M16, lies about 7000 light years away.]]> <![CDATA[Comet Tsuchinshan-ATLAS over California]]> https://apod.nasa.gov/apod/ap241021.htmlhttps://apod.nasa.gov/apod/ap241021.html Brian Fulda Robert Nemiroff (MTU) Jerry Bonnell (UMCP) Mon, 21 Oct 2024 11:00:00 GMT
Explanation: The tails of Comet Tsuchinshan-ATLAS were a sight to behold. Pictured, C/2023 A3 (Tsuchinshan–ATLAS) was captured near peak impressiveness last week over the Eastern Sierra Mountains in California, USA. The comet not only showed a bright tail, but a distinct anti-tail pointing in nearly the opposite direction. The globular star cluster M5 can be seen on the right, far in the distance. As it approached, it was unclear if this crumbling iceberg would disintegrate completely as it warmed in the bright sunlight. In reality, the comet survived to become brighter than any star in the night (magnitude -4.9), but unfortunately was then so nearly in front of the Sun that it was hard for many casual observers to locate. Whether Comet Tsuchinshan-Atlas becomes known as the Great Comet of 2024 now depends, in part, on how impressive incoming comet C/2024 S1 (ATLAS) becomes over the next two weeks.]]> <![CDATA[Dark Matter in a Simulated Universe]]> https://apod.nasa.gov/apod/ap241020.htmlhttps://apod.nasa.gov/apod/ap241020.html Tom Abel Ralf Kaehler KIPAC SLAC AMNH Robert Nemiroff (MTU) Jerry Bonnell (UMCP) Sun, 20 Oct 2024 11:00:00 GMT
Explanation: Is our universe haunted? It might look that way on this dark matter map. The gravity of unseen dark matteris the leading explanation for why galaxies rotate so fast, why galaxies orbit clusters so fast, why gravitational lenses so strongly deflect light, and why visible matter is distributed as it is both in the local universe and on the cosmic microwave background. The featured image from the American Museum of Natural History's Hayden PlanetariumSpace Show Dark Universe highlights one example of how pervasive dark matter might haunt our universe. In this frame from a detailed computer simulation, complex filaments of dark matter, shown in black, are strewn about the universe like spider webs, while the relatively rare clumps of familiar baryonic matter are colored orange.These simulations are good statistical matches to astronomical observations. In what is perhaps a scarier turn of events, dark matter -- although quite strange and in an unknown form -- is no longer thought to be the strangest source of gravity in the universe. That honor now falls to dark energy, a more uniform source of repulsive gravitythat seems to now dominate the expansion of the entire universe.]]> <![CDATA[Comet Tsuchinshan-ATLAS Flys Away]]> https://apod.nasa.gov/apod/ap241019.htmlhttps://apod.nasa.gov/apod/ap241019.html Xingyang Cai Robert Nemiroff (MTU) Jerry Bonnell (UMCP) Sat, 19 Oct 2024 11:00:00 GMT
Explanation: These six panels follow daily apparitions of cometC/2023 A3 Tsuchinshan-ATLASas it moved away from our fair planet during the past week. The images were taken with the same camera and lens at the indicated dates and locations from California, planet Earth. At far right on October 12the visitorfrom the distant Oort cloud was near its closest approach, some 70 million kilometers (about 4 light-minutes) away. Its bright coma and long dust tail were close on the sky to the setting Sun but still easy to spot against a bright western horizon. Over the following days, the outbound comet steadily climbs above the ecliptic and north into the darker western evening sky, but begins to fade from view. Crossing the Earth's orbital plane around October 14, Tsuchinshan-ATLAS exhibits a noticeableantitail extended toward the western horizon. Higher in the evening sky at sunset by October 17 (far left) the comet has faded and reached a distance of around 77 million kilometers from planet Earth.Hopefully you enjoyedsome of Tsuchinshan-ATLAS's bid to become the best comet of 2024.This comet'sinitial orbital period estimates were a mere 80,000 years, butin factit may never return to the inner Solar System.]]> <![CDATA[Most of Comet Tsuchinshan-ATLAS]]> https://apod.nasa.gov/apod/ap241018.htmlhttps://apod.nasa.gov/apod/ap241018.html Adam Block Robert Nemiroff (MTU) Jerry Bonnell (UMCP) Fri, 18 Oct 2024 11:00:00 GMT
Explanation: On October 14 it was hard to capture a full view of Comet C/2023 A3Tsuchinshan-ATLAS. Taken after the comet's closest approach to our fair planet,this evening skyview almost does though. With two telephoto frames combined, the image stretches about 26 degrees across the sky from top to bottom, looking west from Gates Pass, Tucson, Arizona. Comet watchers that night could evenidentifyglobular star cluster M5 and the faint apparition of periodic comet 13P Olbers near the long the path of Tsuchinshan-ATLAS's whitish dust tail above the bright comet's coma.Due to perspectiveas the Earth is crossing the comet's orbital plane, Tsuchinshan-ATLAS also has a pronounced antitail. The antitail is composed of dust previously released and fanning out away from the Sun along the comet's orbit, visible as a needle-like extension below the bright coma toward the rugged western horizon.]]> <![CDATA[The Clipper and the Comet]]> https://apod.nasa.gov/apod/ap241017.htmlhttps://apod.nasa.gov/apod/ap241017.html Ben Cooper Launch Photography Robert Nemiroff (MTU) Jerry Bonnell (UMCP) Thu, 17 Oct 2024 11:00:00 GMT
Explanation: NASA's Europa Clipperis now headed toward an ocean world beyond Earth. The large spacecraft is tucked into the payload fairing atop the Falcon Heavy rocket in thisphoto, taken at Kennedy Space Centerthe day before the mission's successful October 14 launch. Europa Clipper's interplanetary voyage will first take it to Mars, then back to Earth, and then on to Jupiter ongravity assist trajectoriesthat will allow it to enter orbit around Jupiter in April 2030. Once orbiting Jupiter, the spacecraft will fly past Europa 49 times,exploring a Jovian moonwith a global subsurface ocean that may have conditions to support life. Posing in the background next to the floodlit rocket is Comet Tsuchinsan-ATLAS, about a day after the comet's closest approach to Earth. A current darling of evening skies, the naked-eye comet is avisitor from the distant Oort cloud]]> <![CDATA[Colorful Aurora over New Zealand]]> https://apod.nasa.gov/apod/ap241016.htmlhttps://apod.nasa.gov/apod/ap241016.html Tristian McDonald Robert Nemiroff (MTU) Jerry Bonnell (UMCP) Wed, 16 Oct 2024 11:00:00 GMT
Explanation: Sometimes the night sky is full of surprises. Take the sky over Lindis Pass, South Island, New Zealandone-night last week. Instead of a typically calm night sky filled with constant stars, a busy and dynamic night sky appeared. Suddenly visible were pervasive red aurora, green picket-fence aurora, a red SAR arc, a STEVE, a meteor, and the Moon. These outshone the center of our Milky Way Galaxy and both of its two satellite galaxies: the LMC and SMC. All of these were captured together on 28 exposures in five minutes, from which this panorama was composed. Auroras lit up many skies last week, as a Coronal Mass Ejection from the Sun unleashed a burst of particles toward our Earth that created colorful skies over latitudes usually too far from the Earth's poles to see them. More generally, night skies this month have other surprises, showing not only auroras -- but comets.]]> <![CDATA[Animation: Comet Tsuchinshan-ATLAS Tails Prediction]]> https://apod.nasa.gov/apod/ap241015.htmlhttps://apod.nasa.gov/apod/ap241015.html Nico Lefaudeux Robert Nemiroff (MTU) Jerry Bonnell (UMCP) Tue, 15 Oct 2024 11:00:00 GMT
Explanation: How bright and strange will the tails of Comet Tsuchinshan-ATLAS become?The comet has brightened dramatically over the few weeks as it passed its closest to the Sun and, just three days ago, passed its closest to the Earth.C/2023 A3 (Tsuchinshan–ATLAS) became of the brightest comets of the past century over the past few days, but was unfortunately hard to see because it was so nearly superposed on the Sun. As the cometappears to move away from the Sun, it is becoming a remarkable sight -- but may soon begin to fade. The featured animated video shows how the comet's tails have developed, as viewed from Earth, and gives one prediction about how they might further develop. As shown in the video, heavier parts of the dust tail that trails the comet have begun to appear to point in nearly the opposite direction from lighter parts of the dust tail as well as the comet's ion tail, the blue tail that is pushed directly out from the Sun by the solar wind.]]> <![CDATA[Comet Tsuchinshan-ATLAS Over the Lincoln Memorial]]> https://apod.nasa.gov/apod/ap241014.htmlhttps://apod.nasa.gov/apod/ap241014.html Brennan Gilmore Robert Nemiroff (MTU) Jerry Bonnell (UMCP) Mon, 14 Oct 2024 11:00:00 GMT
Explanation: Go outside at sunset tonight and see a comet! C/2023 A3 (Tsuchinshan–ATLAS) has become visible in the early evening sky in northern locations to the unaided eye. To see the comet, look west through a sky with a low horizon. If the sky is clear and dark enough, you will not even need binoculars -- the faint tail of the comet should be visiblejust above the horizon for about an hour. Pictured, Comet Tsuchinshan-ATLAS was captured two nights ago over the Lincoln Memorial monument in Washington, DC, USA. With each passing day at sunset, the cometand its changing tailshould be higher and higher in the sky, although exactly how bright and how long its tails will be can only be guessed.]]> <![CDATA[Aurora Timelapse Over Italian Alps]]> https://apod.nasa.gov/apod/ap241013.htmlhttps://apod.nasa.gov/apod/ap241013.html Cristian Bigontina Robert Nemiroff (MTU) Jerry Bonnell (UMCP) Sun, 13 Oct 2024 11:00:00 GMT
Explanation: Did you see last night's aurora? This question was relevant around much of the world a few days ago because a powerful auroral storm became visible unusually far from the Earth's poles. The cause was a giant X-class solar flare on Tuesdaythat launched energetic electrons and protons into the Solar System, connecting to the Earth via our planet's magnetic field. A red glow of these particles striking oxygen atoms high in Earth's atmosphere pervades the frame, while vertical streaks dance. The featured video shows a one-hour timelapse as seen from Cortina d'Ampezzo over Alps Mountain peaks in northern Italy. Stars from our Milky Way Galaxy dot the background while streaks from airplanes and satellites punctuate the foreground. The high recent activity of our Sun is likely to continue to produce picturesque aurorasover Earth during the next year or so.]]> <![CDATA[Northern Lights, West Virginia]]> https://apod.nasa.gov/apod/ap241012.htmlhttps://apod.nasa.gov/apod/ap241012.html Jonathan Eggleston Robert Nemiroff (MTU) Jerry Bonnell (UMCP) Sat, 12 Oct 2024 11:00:00 GMT
Explanation: A gravel country lane gently winds through thiscolorful ruralnight skyscape. Captured from Monroe County in southern West Virginia on the evening of October 10, the starry sky above is a familiar sight. Shimmering curtains of aurora borealis or northern lights definitely do not make regular appearances here, though. Surprisingly vivid auroral displays were present on that night at very low latitudesaround the globe, far from their usual northern and southernhigh latitude realms. The extensive auroral activity was evidence of a severegeomagnetic stormtriggered by the impact of acoronal mass ejection (CME), an immense magnetized cloud of energetic plasma. The CME was launched toward Earth from the active Sun following a powerfulX-class solar flare.]]> <![CDATA[Ring of Fire over Easter Island]]> https://apod.nasa.gov/apod/ap241011.htmlhttps://apod.nasa.gov/apod/ap241011.html Yuri Beletsky Carnegie Las Campanas Observatory TWAN Robert Nemiroff (MTU) Jerry Bonnell (UMCP) Fri, 11 Oct 2024 11:00:00 GMT
Explanation: The second solar eclipseof 2024 began in the Pacific. On October 2nd the Moon's shadow swept from west to east, with anannular eclipse visiblealong a narrow antumbral shadow path tracking mostly over ocean, making its only major landfall near the southern tip of South America, and then ending in the southern Atlantic. The dramatic total annular eclipse phase is known to some as aring of fire. Also tracking across islands in the southern Pacific, the Moon's antumbral shadow grazed Easter Island allowingdenizens to follow all phases of the annular eclipse. Framed bypalm tree leaves this clear island view is a stack of two images, one taken with and one taken without a solar filter near the moment of the maximum annular phase.The New Moon's silhouetteappears just off center, though still engulfed by the bright disk of the active Sun.]]> <![CDATA[Five Bright Comets from SOHO]]> https://apod.nasa.gov/apod/ap241010.htmlhttps://apod.nasa.gov/apod/ap241010.html Tunc Tezel TWAN Robert Nemiroff (MTU) Jerry Bonnell (UMCP) Thu, 10 Oct 2024 11:00:00 GMT
Explanation: Five bright comets are compared in these panels, recorded by a coronograph on board the long-lived, sun-staringSOHO spacecraft. Arranged chronologically all are recognizable by theirtails streaming awayfrom the Sun at the center of each field of view, where a direct view of the overwhelmingly bright Sun is blocked by the coronagraph's occulting disk. Each comet was memorable for earthbound skygazers, starting at top left withComet McNaught, the 21st century's brightest comet (so far).C/2023 A3 Tsuchinshan-ATLAS, following its perihelion with the active Sun at bottom center, has most recently grabbed the attention of comet watchers around the globe. By the end of October 2024, the blank 6th panel may be filled with bright sungrazer cometC/2024 S1 (ATLAS). ...or not.]]> <![CDATA[M106: A Spiral Galaxy with a Strange Center]]> https://apod.nasa.gov/apod/ap241009.htmlhttps://apod.nasa.gov/apod/ap241009.html Ali Al Obaidly Robert Nemiroff (MTU) Jerry Bonnell (UMCP) Wed, 09 Oct 2024 11:00:00 GMT
Explanation: What's happening at the center of spiral galaxy M106? A swirling disk of stars and gas, M106's appearance is dominated by blue spiral arms and red dust lanes near the nucleus, as shown in the featured imagetaken from the Kuwaiti desert. The core of M106 glows brightly in radio waves and X-rays where twin jets have been found running the length of the galaxy. An unusual central glow makes M106 one of the closest examples of the Seyfert class of galaxies, where vast amounts of glowing gas are thought to be falling into a central massive black hole. M106, also designated NGC 4258, is a relatively close 23.5 million light years away, spans 60 thousand light years across, and can be seen with a small telescope towards the constellation of the Hunting Dogs (Canes Venatici).]]> <![CDATA[Annular Eclipse over Patagonia]]> https://apod.nasa.gov/apod/ap241008.htmlhttps://apod.nasa.gov/apod/ap241008.html Alexis Trigo Robert Nemiroff (MTU) Jerry Bonnell (UMCP) Tue, 08 Oct 2024 11:00:00 GMT
Explanation: Can you find the Sun? OK, but can you explain why there’s a big dark spot in the center? The spot is the Moon, and the impressive alignment shown, where the Moon lines up inside the Sun, is called an annular solar eclipse. Such an eclipse occurred just last week and was visible from a thin swath mostly in Earth's southern hemisphere. The featured image was captured from Patagonia, Chile. When the Moon is significantly closer to the Earth and it aligns with the Sun, a total solar eclipseis then visible from parts of the Earth.Annular eclipses are slightly more common than total eclipses, but as the Moon moves slowly away from the Earth, before a billion more years, the Moon's orbit will no longerbring it close enough for a total solar eclipse to be seen from anywhere on Earth.]]> <![CDATA[The Long Tails Comet Tsuchinshan-ATLAS]]> https://apod.nasa.gov/apod/ap241007.htmlhttps://apod.nasa.gov/apod/ap241007.html Jose Santivañez Mueras Robert Nemiroff (MTU) Jerry Bonnell (UMCP) Mon, 07 Oct 2024 11:00:00 GMT
Explanation: A bright comet is moving into the evening skies.C/2023 A3 (Tsuchinshan–ATLAS) has brightened and even though it is now easily visible to the unaided eye, it is so near to the Sun that it is still difficult to see.Pictured, Comet Tsuchinshan–ATLASwas captured just before sunrise from an Andes Mountain in Peru. Braving cold weather, this unusually high perchgave the astrophotographer such a low eastern horizon that the cometwas obvious in the pre-dawn sky. Visible in the featured image is not only an impressively long dust tail extending over many degrees, but an impressively long and blue ion tail, too. This month, as the comet moves out from the Sunand passes the Earth, evening observers should be able to see the huge dirty ice ball toward the west just after sunset.]]> <![CDATA[The Magnificent Tail of Comet McNaught]]> https://apod.nasa.gov/apod/ap241006.htmlhttps://apod.nasa.gov/apod/ap241006.html Robert H. McNaught Robert Nemiroff (MTU) Jerry Bonnell (UMCP) Sun, 06 Oct 2024 11:00:00 GMT
Explanation: Comet McNaught, the Great Comet of 2007, grew a spectacularly long and filamentary tail. The magnificent tail spread across the sky and was visible for several days to Southern Hemisphere observers just after sunset. The amazing ion tail showed its greatest extent on long-duration, wide-angle camera exposures. During some times, just the tail itself was visible just above the horizon for many northern observers as well.Comet C/2006 P1 (McNaught), estimated to have attained a peak brightness of magnitude -5 (minus five), was caught by the comet's discoverer in the featured image just after sunset in January 2007 from Siding Spring Observatory in Australia. Comet McNaught, the brightest comet in decades, then faded as it moved further into southern skies and away from the Sun and Earth. Over the next month, Comet Tsuchinshan–ATLAS, a candidate for the Great Comet of 2024, should display its most spectacular tailsvisible from the Earth.]]> <![CDATA[M27: Not a Comet]]> https://apod.nasa.gov/apod/ap241005.htmlhttps://apod.nasa.gov/apod/ap241005.html Francesco Sferlazza, Franco Sgueglia Robert Nemiroff (MTU) Jerry Bonnell (UMCP) Sat, 05 Oct 2024 11:00:00 GMT
Explanation: While hunting for comets in the skies above 18th century France,astronomer Charles Messierdiligently kept a list of the things encountered during his telescopic expeditions that were definitely not comets. This is number 27 on hisnow famous not-a-comet list. In fact, 21st century astronomers would identify it as aplanetary nebula, but it's not a planet either, even though it mayappear round and planet-like in a small telescope. Messier 27 (M27) is an excellent example of a gaseous emission nebula created as a sun-like star runs outof nuclear fuel in its core. The nebula forms as the star's outer layers are expelled into space, with a visible glow generated by atoms excited by the dying star's intense but invisibleultraviolet light. Known by the popular name of theDumbbell Nebula, the beautifully symmetric interstellar gas cloud is over 2.5 light-years across and about 1,200 light-years away in theconstellation Vulpecula. This impressive color image highlights details within the well-studied central region and fainter, seldom imaged features in the nebula's outer halo.]]> <![CDATA[Comet at Moonrise]]> https://apod.nasa.gov/apod/ap241004.htmlhttps://apod.nasa.gov/apod/ap241004.html Gabriel Zaparolli Robert Nemiroff (MTU) Jerry Bonnell (UMCP) Fri, 04 Oct 2024 11:00:00 GMT
Explanation: Comet C/2023 A3 (Tsuchinshan–ATLAS)is growing brighter in planet Earth's sky. Fondly known as comet A3, this new visitor to the inner Solar System is traveling from thedistant Oort cloud. The comet reached perihelion, its closest approach to the Sun, on September 27 and will reach perigee, its closest to our fair planet, on October 12, by then becoming an evening sky apparition.But comet A3was an early morning riser on September 30 when this image was made. Its bright coma and already long tail share a pre-dawn skyscape from Praia Grande, Santa Catarina in southern Brazil with the waning crescent Moon just peeking above the eastern horizon. While the behaviour of comets isnotoriouslyunpredictable, Tsuchinshan–ATLAS could become acomet visually rivalingC/2020 F3 (NEOWISE). Comet NEOWISEwowed skygazers in the summer of 2020.]]> <![CDATA[Eclipse at Sunrise]]> https://apod.nasa.gov/apod/ap241003.htmlhttps://apod.nasa.gov/apod/ap241003.html Wang Letian Eyes at Night Robert Nemiroff (MTU) Jerry Bonnell (UMCP) Thu, 03 Oct 2024 11:00:00 GMT
Explanation: The second solar eclipseof 2024 began in the Pacific. On October 2nd the Moon's shadow swept from west to east, with anannular eclipse visible along a narrow antumbral shadow path tracking mostly over ocean, crossing land near the southern tip of South America, and ending in the southern Atlantic. The dramatic total annular eclipse phase is known to some as aring of fire. Still, a partial eclipse of the Sun was experienced over a wide region. Captured at one of its earliest moments, October's eclipsed Sun is seen just above the clouds near sunrise in this snapshot. The partially eclipsed solar disk is close to the maximum eclipse as seen from Mauna Kea Observatory Visitor Center, Island of Hawaii,planet Earth.]]> <![CDATA[The Large Magellanic Cloud Galaxy]]> https://apod.nasa.gov/apod/ap241002.htmlhttps://apod.nasa.gov/apod/ap241002.html Ireneusz Nowak Natalia Lewandowska SUNY Oswego Robert Nemiroff (MTU) Jerry Bonnell (UMCP) Wed, 02 Oct 2024 11:00:00 GMT
Explanation: It is the largest satellite galaxy of our home Milky Way Galaxy. If you live in the south, the Large Magellanic Cloud (LMC) is quite noticeable, spanning about 10 degrees across the night sky, which is 20 times larger than the full moon towards the southern constellation of the dolphinfish(Dorado). Being only about 160,000 light years away, many details of the LMC's structure can be seen, such as its central bar and its single spiral arm. The LMC harbors numerous stellar nurseries where new stars are being born, which appear in pink in the featured image. It is home to the Tarantula Nebula, the currently most active star forming region in the entire Local Group, a small collection of nearby galaxies dominated by the massive Andromeda and Milky Waygalaxies. Studies of the LMC and the Small Magellanic Cloud (SMC) by Henrietta Swan Leavittled to the discovery of the period-luminosity relationship of Cepheid variable stars that are used to measure distances across the nearby universe.]]> <![CDATA[Porphyrion: The Longest Known Black Hole Jets]]> https://apod.nasa.gov/apod/ap241001.htmlhttps://apod.nasa.gov/apod/ap241001.html Science Communication Lab Martijn Oei et al. Caltech Robert Nemiroff (MTU) Jerry Bonnell (UMCP) Tue, 01 Oct 2024 11:00:00 GMT
Explanation: How far can black hole jets extend? A new record was foundjust recently with the discovery of a 23-million light-year long jet pair from a black hole active billions of years ago. Dubbed Porphyrion for a mythological Greek giant, the impressive jets were created by a type of black hole that does not usually create long jets -- one that is busy creating radiation from infalling gas. The featured animated videodepicts what it might look like to circle around this powerful black holesystem. Porphyrion is shown as a fast stream of energetic particles, and the bright areas are where these particles are impacting surrounding gas. The discovery was made using data from the Keck and Mayall(DESI) optical observatories as well as LOFARand the Giant Metrewave Radio Telescope. The existence of these jets demonstrates that black holes can affect not only their home galaxies but far out into the surrounding universe.]]> <![CDATA[Comet Tsuchinshan-ATLAS over Mexico]]> https://apod.nasa.gov/apod/ap240930.htmlhttps://apod.nasa.gov/apod/ap240930.html Daniel Korona Robert Nemiroff (MTU) Jerry Bonnell (UMCP) Mon, 30 Sep 2024 11:00:00 GMT
Explanation: The new comet has passed its closest to the Sun and is now moving closer to the Earth.C/2023 A3 (Tsuchinshan–ATLAS) is currently moving out from inside the orbit of Venus and on track to pass its nearest to the Earth in about two weeks. Comet Tsuchinshan-ATLAS, pronounced "Choo-cheen-shahn At-less,", is near naked-eye visibility and easily picked up by long-exposure cameras. The comet can also now be found by observers in Earth's northern hemisphere as well as the south. The featured image was captured just a few days ago above Zacatecas, Mexico. Because clouds were obscuring much of the pre-dawn sky, the astrophotographer released a drone to take pictures from higher up, several of which were later merged to enhance the comet's visibility. Although the future brightness of comets is hard to predict, there is increasing hope that Comet Tsuchinshan-ATLASwill further brighten as it enters the early evening sky.]]> <![CDATA[Seven Dusty Sisters]]> https://apod.nasa.gov/apod/ap240929.htmlhttps://apod.nasa.gov/apod/ap240929.html WISE IRSA NASA Francesco Antonucci Robert Nemiroff (MTU) Jerry Bonnell (UMCP) Sun, 29 Sep 2024 11:00:00 GMT
Explanation: Is this really the famous Pleiades star cluster? Known for its iconic blue stars, the Pleiades is shown here in infrared lightwhere the surrounding dust outshines the stars. Here, three infrared colors have been mapped into visual colors (R=24, G=12, B=4.6 microns). The base images were taken by NASA's orbiting Wide Field Infrared Survey Explorer (WISE) spacecraft. Cataloged as M45 and nicknamed the Seven Sisters, the Pleiadesstar cluster is by chance situated in a passing dust cloud. The light and winds from the massive Pleiades stars preferentially repel smaller dust particles, causing the dust to become stratified into filaments, as seen. The featured image spans about 20 light years at the distance of the Pleiades, which lies about 450 light years distant toward the constellation of the Bull (Taurus).]]> <![CDATA[Rocket Eclipse at Sunset]]> https://apod.nasa.gov/apod/ap240928.htmlhttps://apod.nasa.gov/apod/ap240928.html Ben Cooper Launch Photography Robert Nemiroff (MTU) Jerry Bonnell (UMCP) Sat, 28 Sep 2024 11:00:00 GMT
Explanation: Shockwaves ripple across the glare as a launch eclipses the setting Sun in thisexciting close-up. Captured on September 17, the roaring Falcon 9 rocket carried European Galileo L13 navigation satellites to medium Earth orbitafter a lift-offfrom Cape Canaveral on Florida's space coast. The Falcon 9 booster returned safely to Earth about 8.5 minutes later, notching the 22nd launch _and_landing for the reusable workhorse launch vehicle. But where did it land?Just Read the Instructions.]]> <![CDATA[Stellar Streams in the Local Universe]]> https://apod.nasa.gov/apod/ap240927.htmlhttps://apod.nasa.gov/apod/ap240927.html David Martinez Delgado et al. Robert Nemiroff (MTU) Jerry Bonnell (UMCP) Fri, 27 Sep 2024 11:00:00 GMT
Explanation: The twenty galaxiesarrayed in these panels are part of an ambitious astronomical survey of tidal stellar streams. Each panel presents a composite view; a deep, inverted image taken from publiclyavailable imaging surveysof a field that surrounds anearby massive galaxy image. The inverted images reveal faint cosmic structures, star streams hundreds of thousands of light-years across, that result from the gravitational disruption andeventual merger of satellite galaxiesin thelocal universe. Such surveys of mergers and gravitational tidal interactions between massive galaxies and their dwarf satellites arecrucial guides for current models of galaxy formation and cosmology. Of course, the detection of stellar streams in the neighboring Andromeda Galaxy andour own Milky Wayalso offers spectacular evidence for ongoing satellite galaxy disruption within our morelocal galaxy group.]]> <![CDATA[The Great Globular Cluster in Hercules]]> https://apod.nasa.gov/apod/ap240926.htmlhttps://apod.nasa.gov/apod/ap240926.html Jan Beckmann, Julian Zoller, Lukas Eisert, Wolfgang Hummel Robert Nemiroff (MTU) Jerry Bonnell (UMCP) Thu, 26 Sep 2024 11:00:00 GMT
Explanation: In 1716, English astronomerEdmond Halleynoted, "This is but a little Patch, but it shows itself to the naked Eye, when the Sky is serene and the Moon absent."Of course, M13is now less modestly recognized as the Great Globular Cluster in Hercules, one of the brightestglobular star clusters in the northern sky. Sharp telescopic views like this one reveal the spectacular cluster'shundreds of thousands of stars.At a distance of 25,000 light-years, thecluster stars crowdinto a region 150 light-years in diameter.Approaching the cluster core, upwards of 100 stars could be contained in a cube just 3 light-years on a side. For comparison, theclosest star to the Sun is over 4 light-years away. The deep, wide-field image also reveals distant background galaxies including NGC 6207 at the upper left, and faint, foreground Milky Way dust clouds known to some as integrated flux nebulae.]]> <![CDATA[Comet A3 Through an Australian Sunrise]]> https://apod.nasa.gov/apod/ap240925.htmlhttps://apod.nasa.gov/apod/ap240925.html Lucy Yunxi Hu Robert Nemiroff (MTU) Jerry Bonnell (UMCP) Wed, 25 Sep 2024 11:00:00 GMT
Explanation: Comet Tsuchinshan-ATLAS is now visible in the early morning sky. Diving into the inner Solar System at an odd angle, this large dirty iceberg will pass its closest to the Sun -- between the orbits of Mercury and Venus -- in just two days. Long camera exposures are now capturing C/2023 A3 (Tsuchinshan–ATLAS), sometimes abbreviated as just A3, and its dust tail before and during sunrise. The featured image composite was taken four days ago and captured the comet as it rose above Lake George, NSW, Australia. Vertical bands further left are images of the comet as the rising Sun made the predawn sky increasingly bright and colorful. Just how bright the comet will become over the next month is currently unknown as it involves how much gas and dust the comet's nucleus will expel. Optimistic skywatchers are hopingfor a great show where Tsuchinshan–ATLAS creates dust and ion tails visible across Earth's sky and becomes known as the Great Comet of 2024.]]> <![CDATA[NGC 6727: The Rampaging Baboon Nebula]]> https://apod.nasa.gov/apod/ap240924.htmlhttps://apod.nasa.gov/apod/ap240924.html Alpha Zhang Ting Yu Robert Nemiroff (MTU) Jerry Bonnell (UMCP) Tue, 24 Sep 2024 11:00:00 GMT
Explanation: This dusty region is forming stars. Part of a sprawling molecular cloudcomplex that resembles, to some, a rampaging baboon, the region is a relatively close by 500 light-years away toward the constellationCorona Australis. That's about one third the distance of the more famous stellar nursery known as the Orion Nebula. Mixed with bright nebulosities, the brown dust clouds effectively block light from more distant background stars in the Milky Way and obscure from viewembedded stars still in the process of formation. The eyes of the dust creature in the featured image are actually blue reflection nebulas cataloged as NGC 6726, 6727, 6729, and IC 4812, while the red mouth glows with light emitted by hydrogen gas. Just to the upper left of the baboon's head is NGC 6723, a whole globular clusterof stars nearly 30,000 light years in the distance.]]> <![CDATA[Comet Tsuchinshan-ATLAS Approaches]]> https://apod.nasa.gov/apod/ap240923.htmlhttps://apod.nasa.gov/apod/ap240923.html Brian Valente Robert Nemiroff (MTU) Jerry Bonnell (UMCP) Mon, 23 Sep 2024 11:00:00 GMT
Explanation: What will happen as this already bright comet approaches? Optimistic predictions have Comet C/2023 A3 (Tsuchinshan–ATLAS) briefly becoming easily visible to the unaided eye -- although the future brightness of comets are notoriously hard to predict, and this comet may even break up in warming sunlight. What is certain is that the comet is now unexpectedly bright and is on trackto pass its closest to the Sun (0.39 AU) later this week and closest to the Earth(0.47 AU) early next month. The featured imagewas taken in late May as Comet Tsuchinshan–ATLAS, discovered only last year, passed nearly in front of two distant galaxies. The comet can now be found with binoculars in the early morning sky rising just before the Sun, while over the next few weeks it will brightenas it moves to the early evening sky.]]> <![CDATA[Chicagohenge: Equinox in an Aligned City]]> https://apod.nasa.gov/apod/ap240922.htmlhttps://apod.nasa.gov/apod/ap240922.html Anthony Artese Robert Nemiroff (MTU) Jerry Bonnell (UMCP) Sun, 22 Sep 2024 11:00:00 GMT
Explanation: Chicago, in a way, is like a modern Stonehenge. The way is east to west, and the time is today. Today, and every equinox, theSunwill set exactly to the west, everywhere on Earth. Therefore, today in Chicago, the Sun will set directly down the long equatorially-aligned grid of streets and buildings, an event dubbed #chicagohenge. Featured here is a Chicago Hengepicture taken during the equinoxin mid-September of 2017 looking along part of Upper Wacker Drive. Many cities, though, have streets or other features that are well-aligned to Earth's spin axis. Therefore, quite possibly, your favorite street may also run east - west. Tonight at sunset, with a quick glance, you can actually find out.]]> <![CDATA[Sunrise Shadows in the Sky]]> https://apod.nasa.gov/apod/ap240921.htmlhttps://apod.nasa.gov/apod/ap240921.html Emili Vilamala Robert Nemiroff (MTU) Jerry Bonnell (UMCP) Sat, 21 Sep 2024 11:00:00 GMT
Explanation: The defining astronomical momentof this September's equinox is at 12:44 UTC on September 22, when the Sun crosses the celestial equator moving south in itsyearly journey through planet Earth's sky. That marks the beginning offall for our fair planetin the northern hemisphere and spring in the southern hemisphere, when day and night are nearly equal around the globe. Of course, if you celebrate the astronomical change of seasons by watching a sunrise you can alsolook for crepuscular rays. Outlined by shadows cast by clouds, crepuscular rays can have a dramatic appearance in the twilight sky during any sunrise (or sunset). Due to perspective, the parallel cloud shadows will seem to point back to the rising Sunand a placedue east on your horizon on the equinox date. But in this spectacular sunrise skyscape captured in early June, the parallel shadows and crepuscular rays appear to converge toward an eastern horizon's more northerly sunrise. The well-composed photo places the rising Sun just behind the bell tower of a church in the town of Vic, province of Barcelona, Catalonia, Spain.]]> <![CDATA[A Hazy Harvest Moon]]> https://apod.nasa.gov/apod/ap240920.htmlhttps://apod.nasa.gov/apod/ap240920.html Petr Horálek Institute of Physics in Opava Robert Nemiroff (MTU) Jerry Bonnell (UMCP) Fri, 20 Sep 2024 11:00:00 GMT
Explanation: For northern hemisphere dwellers, September's Full Moon wasthe Harvest Moon. On September 17/18 the sunlit lunar nearside passed into shadow, just grazing Earth's umbra, the planet's dark, central shadow cone, in apartial lunar eclipse. Over the two and a half hours before dawn a camera fixed to a tripod was used to record thisseries of exposuresas the eclipsed Harvest Moon set behind Spiš Castle in the hazy morning sky over eastern Slovakia. Famed in festival, story, and song, Harvest Moon is just the traditional name of the full moon nearest theautumnalequinox. According to lore the name is a fitting one. Despite the diminishing daylight hours as thegrowing seasondrew to a close, farmers could harvest crops by the light of a full moonshining onfrom dusk to dawn. This September's Harvest Moon was also known to some as a supermoon, a term becoming a traditional name for afull moon near perigee.]]> <![CDATA[The Dark Seahorse of Cepheus]]> https://apod.nasa.gov/apod/ap240919.htmlhttps://apod.nasa.gov/apod/ap240919.html Davide Broise Robert Nemiroff (MTU) Jerry Bonnell (UMCP) Thu, 19 Sep 2024 11:00:00 GMT
Explanation: Spanning light-years, thissuggestiveshape known as the Seahorse Nebula floats in silhouette against a rich, luminous background of stars. Seen toward the royal northern constellation of Cepheus, the dusty, dark nebula is part of a Milky Way molecular cloud some 1,200 light-years distant. It is also listed as Barnard 150 (B150), one of 182dark markings of the skycataloged in the early 20th century by astronomerE. E. Barnard. Packs of low mass stars are formingwithin, but their collapsing cores are only visible at longinfrared wavelengths. Still, the colorful Milky Way stars of Cepheus add to this stunninggalactic skyscape.]]>