View allAll Photos Tagged solarsystemandbeyond
Astronomers have detected X-rays from Uranus for the first time, using NASA’s Chandra X-ray Observatory. This result may help scientists learn more about this enigmatic ice giant planet in our solar system.
Uranus is the seventh planet from the Sun and has two sets of rings around its equator. The planet, which has four times the diameter of Earth, rotates on its side, making it different from all other planets in the solar system. Since Voyager 2 was the only spacecraft to ever fly by Uranus, astronomers currently rely on telescopes much closer to Earth, like Chandra and the Hubble Space Telescope, to learn about this distant and cold planet that is made up almost entirely of hydrogen and helium.
In the new study, researchers used Chandra observations taken in Uranus in 2002 and then again in 2017. They saw a clear detection of X-rays from the first observation, just analyzed recently, and a possible flare of X-rays in those obtained fifteen years later. The main graphic shows a Chandra X-ray image of Uranus from 2002 (in pink) superimposed on an optical image from the Keck-I Telescope obtained in a separate study in 2004. The latter shows the planet at approximately the same orientation as it was during the 2002 Chandra observations.
What could cause Uranus to emit X-rays? The answer: mainly the Sun. Astronomers have observed that both Jupiter and Saturn scatter X-ray light given off by the Sun, similar to how Earth’s atmosphere scatters the Sun’s light. While the authors of the new Uranus study initially expected that most of the X-rays detected would also be from scattering, there are tantalizing hints that at least one other source of X-rays is present. If further observations confirm this, it could have intriguing implications for understanding Uranus.
One possibility is that the rings of Uranus are producing X-rays themselves, which is the case for Saturn’s rings. Uranus is surrounded by charged particles such as electrons and protons in its nearby space environment. If these energetic particles collide with the rings, they could cause the rings to glow in X-rays. Another possibility is that at least some of the X-rays come from auroras on Uranus, a phenomenon that has previously been observed on this planet at other wavelengths.
Image credit: X-ray: NASA/CXO/University College London/W. Dunn et al; Optical: W.M. Keck Observatory
#NASA #MarshallSpaceFlightCenter #MSFC #Marshall #chandraxrayobservatory #ChandraXRay #cxo #chandra #astronomy #space #astrophysics #nasamarshallspaceflightcenter #solarsystemandbeyond #planet #uranus
This unusual lenticular galaxy, which is between a spiral and elliptical shape, has lost almost all the gas and dust from its signature spiral arms, which used to orbit around its center. Known as NGC 1947, this galaxy was discovered almost 200 years ago by James Dunlop, a Scottish-born astronomer who later studied the sky from Australia. NGC 1947 can only be seen from the southern hemisphere, in the constellation Dorado (the Dolphinfish).
Residing around 40 million light-years away from Earth, this galaxy shows off its structure by backlighting its remaining faint gas and dust disk with millions of stars. In this picture, taken with the NASA/ESA Hubble Space Telescope, the faint remnants of the galaxy’s spiral arms can still be made out in the stretched thin threads of dark gas encircling it. Without most of its star-forming material, it is unlikely that many new stars will be born within NGC 1947, leaving this galaxy to continue fading with time.
Image credit: ESA/Hubble & NASA, D. Rosario; Acknowledgment: L. Shatz
#NASA #MarshallSpaceFlightCenter #MSFC #Marshall #HubbleSpaceTelescope #HST #astronomy #space #astrophysics #solarsystemandbeyond #gsfc #Goddard #GoddardSpaceFlightCenter #ESA #EuropeanSpaceAgency #galaxy
This image from the NASA/ESA Hubble Space Telescope features the spectacular galaxy NGC 2442, nicknamed the Meathook galaxy owing to its extremely asymmetrical and irregular shape.
This galaxy was host to a supernova explosion spotted in March 2015, known as SN 2015F, that was created by a white dwarf star. The white dwarf was part of a binary star system and siphoned mass from its companion, eventually becoming too greedy and taking on more than it could handle. This unbalanced the star and triggered runaway nuclear fusion that eventually led to an intensely violent supernova explosion. The supernova shone brightly for quite some time and was easily visible from Earth through even a small telescope until months later.
Image Credit: ESA/Hubble & NASA, S. Smartt et al.
#NASA #MarshallSpaceFlightCenter #MSFC #Marshall #HubbleSpaceTelescope #HST #astronomy #space #astrophysics #Goddard #GoddardSpaceFlightCenter #ESA #EuropeanSpaceAgency #galaxy #supernova #solarsystemandbeyond #gsfc
NGC 6891 is a bright, asymmetrical planetary nebula in the constellation Delphinus, the Dolphin. This Hubble image reveals a wealth of structure, including a spherical outer halo that is expanding faster than the inner nebula, and at least two ellipsoidal shells that are orientated differently. The image also reveals filaments and knots in the nebula’s interior, surrounding the central white dwarf star. From their motions, astronomers estimate that one of the shells is 4,800 years old while the outer halo is some 28,000 years old, indicating a series of outbursts from the dying star at different times.
Hubble studied NGC 6891 as part of efforts to gauge the distances to nebulae, and to learn more about how their structures formed and evolved. NGC 6891 is made up of gas that’s been ionized by the central white dwarf star, which stripped electrons from the nebula’s hydrogen atoms. As the energized electrons revert from their higher-energy state to a lower-energy state by recombining with the hydrogen nuclei, they emit energy in the form of light, causing the nebula’s gas to glow.
Image Credit: NASA, ESA, A. Hajian (University of Waterloo), H. Bond (Pennsylvania State University), and B. Balick (University of Washington); Processing: Gladys Kober (NASA/Catholic University of America)
#NASA #MarshallSpaceFlightCenter #MSFC #Marshall #HubbleSpaceTelescope #HST #astronomy #space #astrophysics #solarsystemandbeyond #gsfc #Goddard #GoddardSpaceFlightCenter #ESA #EuropeanSpaceAgency #nebula #absorptionnebula
This NASA/ESA Hubble Space Telescope image features two interacting galaxies that are so intertwined, they have a collective name – Arp 91. Their delicate galactic dance takes place more than 100 million light-years from Earth. The two galaxies comprising Arp 91 have their own names: the lower galaxy, which looks like a bright spot, is NGC 5953, and the oval-shaped galaxy to the upper right is NGC 5954. In reality, both of them are spiral galaxies, but their shapes appear very different because of their orientation with respect to Earth.
Arp 91 provides a particularly vivid example of galactic interaction. NGC 5953 is clearly tugging at NGC 5954, which looks like it is extending one spiral arm downward. The immense gravitational attraction of the two galaxies is causing them to interact. Such gravitational interactions are common and an important part of galactic evolution. Most astronomers think that collisions between spiral galaxies lead to the formation of another type of galaxy, known as elliptical galaxies. These extremely energetic and massive collisions, however, happen on timescales that dwarf a human lifetime. They take place over hundreds of millions of years, so we should not expect Arp 91 to look any different over the course of our lifetimes!
Image credit: ESA/Hubble & NASA, J. Dalcanton; Acknowledgment: J. Schmidt
#NASA #MarshallSpaceFlightCenter #MSFC #Marshall #HubbleSpaceTelescope #HST #astronomy #space #astrophysics #solarsystemandbeyond #gsfc #Goddard #GoddardSpaceFlightCenter #ESA #EuropeanSpaceAgency #galaxy #EinsteinRing #gravitationallensing
This is the first high-resolution, color image to be sent back by the Hazard Cameras on the underside of NASA’s Perseverance Mars rover after its landing on Feb. 18, 2021.
Video from landing chronicles major milestones during the final minutes of its entry, descent, and landing on the Red Planet, as the spacecraft plummeted, parachuted, and rocketed toward the surface of Mars. A microphone on the rover also has provided the first audio recording of sounds from Mars.
From the moment of parachute inflation, the camera system covers the entirety of the descent process, showing some of the rover’s intense ride to Mars’ Jezero Crater. The footage from high-definition cameras aboard the spacecraft starts 7 miles (11 kilometers) above the surface, showing the supersonic deployment of the most massive parachute ever sent to another world, and ends with the rover’s touchdown in the crater.
Image Credit: NASA/JPL-Caltech
#NASA #jpl #jetpropulsionlaboratory #marshallspaceflightcenter #msfc #mars #moontomars #planet #space #CountdownToMars
This image features the spiral galaxy NGC 691, imaged in fantastic detail using Hubble’s Wide Field Camera 3 (WFC3). This galaxy is a member of the NGC 691 galaxy group named after it, which features a group of gravitationally bound galaxies that lie about 120 million light-years from Earth.
Hubble observes objects such as NGC 691 using a range of filters. Each filter only allows certain wavelengths of light to reach Hubble’s WFC3. The resulting filtered images are colored by specialists who make informed choices about which color best corresponds to the wavelengths of light from the astronomical object that are transmitted by each filter. Combining the colored images from individual filters creates a full-color image. This detailed process provides us with remarkably good insight into the nature and appearance of these objects.
Image credit: ESA/Hubble & NASA, A. Riess et al.; Acknowledgment: M. Zamani
#NASA #MarshallSpaceFlightCenter #MSFC #Marshall #HubbleSpaceTelescope #HST #astronomy #space #astrophysics #solarsystemandbeyond #gsfc #Goddard #GoddardSpaceFlightCenter #ESA #EuropeanSpaceAgency #galaxy
Located in the constellation of Virgo (The Virgin), around 50 million light-years from Earth, the galaxy NGC 4535 is truly a stunning sight to behold. Despite the incredible quality of this image, taken from the NASA/ESA Hubble Space Telescope, NGC 4535 has a hazy, somewhat ghostly, appearance when viewed from a smaller telescope. This led amateur astronomer Leland S. Copeland to nickname NGC 4535 the “Lost Galaxy” in the 1950s.
The bright colors in this image aren’t just beautiful to look at, as they actually tell us about the population of stars within this barred spiral galaxy. The bright blue-ish colors, seen nestled amongst NGC 4535’s long, spiral arms, indicate the presence of a greater number of younger and hotter stars. In contrast, the yellower tones of this galaxy’s bulge suggest that this central area is home to stars which are older and cooler.
This galaxy was studied as part of the Physics at High Angular resolution in Nearby GalaxieS (PHANGS) survey, which aims to clarify many of the links between cold gas clouds, star formation, and the overall shape and other properties of galaxies. On January 11, 2021 the first release of the PHANGS-HST Collection was made publicly available.
Image credit: ESA/Hubble & NASA, J. Lee and the PHANGS-HST Team
#NASA #MarshallSpaceFlightCenter #MSFC #Marshall #HubbleSpaceTelescope #HST #astronomy #space #astrophysics #solarsystemandbeyond #gsfc #Goddard #GoddardSpaceFlightCenter #galaxy
Galaxy clusters are the largest objects in the universe held together by gravity. They contain enormous amounts of superheated gas, with temperatures of tens of millions of degrees, which glows brightly in X-rays, and can be observed across millions of light years between the galaxies. This image of the Abell 2744 galaxy cluster combines X-rays from Chandra (diffuse blue emission) with optical light data from Hubble (red, green, and blue).
Image credit: NASA/CXC; Optical: NASA/STScI
#NASA #MarshallSpaceFlightCenter #MSFC #Marshall #chandraxrayobservatory #ChandraXRay #cxo #chandra #astronomy #space #astrophysics #nasamarshallspaceflightcenter #solarsystemandbeyond #galaxy #galaxycluster #GoddardSpaceFlightCenter #GSFC #Hubble #HST #HubbleSpaceTelescope
Two enormous galaxies capture your attention in this spectacular image taken with the NASA/ESA Hubble Space Telescope using the Wide Field Camera 3 (WFC3). The galaxy on the left is a lenticular galaxy, named 2MASX J03193743+4137580. The side-on spiral galaxy on the right is more simply named UGC 2665. Both galaxies lie approximately 350 million light-years from Earth, and they both form part of the huge Perseus galaxy cluster.
Perseus is an important figure in Greek mythology, renowned for slaying Medusa the Gorgon – who is herself famous for the unhappy reason that she was cursed to have living snakes for hair. Given Perseus’s impressive credentials, it seems appropriate that the galaxy cluster is one of the biggest objects in the known universe, consisting of thousands of galaxies, only a few of which are visible in this image. The wonderful detail in the image is thanks to the WFC3’s powerful resolution and sensitivity to both visible and near-infrared light, the wavelengths captured in this image.
Image credit: ESA/Hubble & NASA, W. Harris; Acknowledgment: L. Shatz
#NASA #MarshallSpaceFlightCenter #MSFC #Marshall #HubbleSpaceTelescope #HST #astronomy #space #astrophysics #solarsystemandbeyond #gsfc #Goddard #GoddardSpaceFlightCenter #ESA #EuropeanSpaceAgency #galaxy
New findings from NASA’s Juno probe orbiting Jupiter provide a fuller picture of how the planet’s distinctive and colorful atmospheric features offer clues about the unseen processes below its clouds. The results highlight the inner workings of the belts and zones of clouds encircling Jupiter, as well as its polar cyclones and even the Great Red Spot.
Jupiter's banded appearance is created by the cloud-forming weather layer. This composite image shows views of Jupiter in infrared and visible light taken by the Gemini North telescope and NASA's Hubble Space Telescope.
Credits: International Gemini Observatory/NOIRLab/NSF/AURA/NASA/ESA, M.H. Wong and I. de Pater (UC Berkeley) et al.
#NASA #MarshallSpaceFlightCenter #MSFC #Marshall #jpl #jetpropulsionlaboratory #nasamarshall #MSFC #solarsystem #juno #jupiter #space #astronomy #nasajuno #nasamarshallspaceflightcenter #HubbleSpaceTelescope #HST #ESA #EuropeanSpaceAgency
NASA’s Juno mission captured these elaborate atmospheric jets in Jupiter's northern mid-latitude region. This detailed, color-enhanced image reveals a complex topography in Jupiter’s cloud tops. If you look closely, relatively small, bright, “pop-up” clouds — which rise above the surrounding features — stand out at the tops and edges of the swirling patterns, while the darker areas nearby reveal greater depth.
Citizen scientist Kevin M. Gill processed this JunoCam image, which was taken on April 10, 2020, at 6:37 a.m. PDT (9:37 a.m. EDT), as the Juno spacecraft performed its 26th close flyby of the planet. At the time the image was taken, the spacecraft was about 5,375 miles (8,650 kilometers) from Jupiter’s cloud tops at a latitude of about 50 degrees North. The spacecraft was traveling about 127,000 mph (204,000 kilometers per hour) relative to the planet at that time.
Image Credit: Image data: NASA/JPL-Caltech/SwRI/MSSS Image processing by Kevin M. Gill © CC BY
NASA’s Curiosity Mars rover used two different cameras to create this selfie in front of Mont Mercou, a rock outcrop that stands 20 feet (6 meters) tall. The panorama is made up of 60 images taken by the Mars Hand Lens Imager (MAHLI) on the rover’s robotic arm on March 26, 2021, the 3,070th Martian day, or sol, of the mission. These were combined with 11 images taken by the Mastcam on the mast, or “head,” of the rover on March 16, 2021, the 3,060th Martian day of the mission.
The hole visible to the left of the rover is where its robotic drill sampled a rock nicknamed “Nontron.” The Curiosity team is nicknaming features in this part of Mars using names from the region around the village of Nontron in southwestern France.
Curiosity was built by NASA’s Jet Propulsion Laboratory in Southern California. Caltech in Pasadena, California, manages JPL for NASA. JPL manages Curiosity's mission for NASA’s Science Mission Directorate in Washington. MAHLI was built by Malin Space Science Systems in San Diego.
Image Credit: NASA/JPL-Caltech
#NASA #jpl #jetpropulsionlaboratory #marshallspaceflightcenter #msfc #mars #moontomars #planet #space #curiosity #MarsScienceLaboratory #MarsCuriosityRover #curiosityrover
Lighting from two times of day was combined for a stunning view of terrain that the rover is leaving behind.
After completing a major software update in April, NASA’s Curiosity Mars rover took a last look at “Marker Band Valley” before leaving it behind, capturing a “postcard” of the scene.
The postcard is an artistic interpretation of the landscape, with color added over two black-and-white panoramas captured by Curiosity’s navigation cameras. The views were taken on April 8 at 9:20 a.m. and 3:40 p.m. local Mars time, providing dramatically different lighting that, when combined, makes details in the scene stand out. Blue was added to parts of the postcard captured in the morning and yellow to parts taken in the afternoon, just as with a similar postcard taken by Curiosity in November 2021.
The resulting image is striking. Curiosity is in the foothills of Mount Sharp, which stands 3 miles (5 kilometers) high within Gale Crater, where the rover has been exploring since landing in 2012. In the distance beyond its tracks is Marker Band Valley, a winding area in the “sulfate-bearing region” within which the rover discovered unexpected signs of an ancient lake. Farther below (at center and just to the right) are two hills – “Bolívar” and “Deepdale” – that Curiosity drove between while exploring “Paraitepuy Pass.”
Image Credit: NASA
#NASA #moontomars #MarsScienceLaboratory #MarsCuriosityRover #curiosityrover
This enhanced-color image from NASA’s Juno spacecraft captures the striking cloud bands of Jupiter’s southern latitudes. Jupiter is not only the largest planet in the solar system, it also rotates at the fastest rate, completing a full day in just 10 hours. This rapid spinning creates strong jet streams, separating Jupiter’s clouds into bright zones and dark belts that wrap around the planet.
Citizen scientist David Marriott created this image with data from the JunoCam instrument. The original image was taken on April 10, 2020, at 7:35 a.m. PDT (10:35 a.m. EDT) as the Juno spacecraft performed its 26th close flyby of the planet. At the time the image was taken, Juno was about 40,000 miles (64,000 kilometers) from the planet’s cloud tops at a latitude of about 58 degrees south.
Image Credit: Image data: NASA/JPL-Caltech/SwRI/MSSS; Image processing by David Marriott
During its 40th close pass by Jupiter, our Juno spacecraft saw Ganymede cast a large, dark spot on the planet on Feb. 25, 2022.
JunoCam captured this image from very close to Jupiter, making Ganymede’s shadow appear especially large. At the time the raw image was taken, the Juno spacecraft was about 44,000 miles (71,000 kilometers) above Jupiter’s cloud tops and 15 times closer to the planet than Ganymede.
An observer at Jupiter’s cloud tops within the oval shadow would experience a total eclipse of the Sun. Total eclipses are more common on Jupiter than Earth for several reasons: Jupiter has four major moons (Ganymede, Io, Callisto, and Europa) that often pass between Jupiter and the Sun, and since Jupiter’s moons orbit in a plane close to Jupiter’s orbital plane, the moon shadows are often cast upon the planet.
Image Credit: Data: NASA/JPL-Caltech/SwRI/MSSS; Image processing: Thomas Thomopoulos © CC BY
#NASA #MarshallSpaceFlightCenter #MSFC #Marshall #jpl #jetpropulsionlaboratory #nasamarshall #juno #nasajuno #ganymede
A blue halo glows around Pluto’s receding crescent in this parting image taken by NASA's New Horizons spacecraft on July 14, 2015. At the time of this shot, New Horizons was 120,000 miles (200,000 kilometers) away from Pluto.
Shown in approximate true color, the picture was constructed from a mosaic of six black-and-white images from the Long Range Reconnaissance Imager, with color added from a lower resolution Ralph/Multispectral Visible Imaging Camera color image.
Scientists believe the haze is a smog resulting from the action of sunlight on methane and other molecules in Pluto's atmosphere. This reaction produces a complex mixture of hydrocarbons that accumulate into small haze particles which scatter blue light. As they settle down through the atmosphere, the haze particles form numerous intricate horizontal layers that extend to altitudes of over 120 miles (200 kilometers).
Image Credit: NASA/Johns Hopkins University Applied Physics Laboratory/Southwest Research Institute
#NASA #NASAMarshall #NASAMarshallSpaceFlightCenter #MSFC #NewHorizons #SolarSystemandBeyond #Pluto #marshallspaceflightcenter #NewFrontiers
This high-resolution still image is part of a video taken by several cameras as NASA’s Perseverance rover touched down on Mars on Feb. 18, 2021. A camera aboard the descent stage captured this shot. A key objective for Perseverance’s mission on Mars is astrobiology, including the search for signs of ancient microbial life. The rover will characterize the planet’s geology and past climate, pave the way for human exploration of the Red Planet, and be the first mission to collect and cache Martian rock and regolith (broken rock and dust). Subsequent NASA missions, in cooperation with ESA (the European Space Agency), would send spacecraft to Mars to collect these cached samples from the surface and return them to Earth for in-depth analysis. The Mars 2020 mission is part of a larger program that includes missions to the Moon as a way to prepare for human exploration of the Red Planet. JPL, which is managed for NASA by Caltech in Pasadena, California, built and manages operations of the Perseverance and Curiosity rovers.
Image Credit: NASA/JPL-Caltech
#NASA #jpl #jetpropulsionlaboratory #marshallspaceflightcenter #msfc #mars #moontomars #planet #space #CountdownToMars
The first of two solar arrays for NASA’s Psyche spacecraft has been extended inside the Astrotech Space Operations Facility near the agency’s Kennedy Space Center in Florida on July 20, 2023.
This week, NASA invited media to view the Psyche spacecraft at 9 a.m. EDT Friday, Aug. 11, at the Astrotech Space Operations payload processing facility in Titusville, Florida.
The Psyche mission is a journey to a metal-rich asteroid orbiting the Sun between Mars and Jupiter. What makes the asteroid Psyche unique is that it appears to be exposed nickel-iron core material of an early planetesimal, one of the building blocks of our solar system.
Deep within rocky, terrestrial planets – including Earth – scientists infer the presence of metallic cores, but these lie unreachably far below the planets' rocky mantles and crusts. Because we cannot see or measure Earth's core directly, Psyche offers a unique window into the violent history of collisions and accretion that created the terrestrial planets.
DSOC will be NASA’s furthest-ever test of high-bandwidth optical communications. DSOC will send and receive test data from Earth using an invisible near-infrared laser, which can transmit data at 10 to 100 times the bandwidth of conventional radio wave systems used on spacecraft today. As the first demonstration of deep-space laser communications, DSOC is not relaying mission data from Psyche. Although, what the team learns from DSOC could support future agency missions, including humanity's next giant leap: When NASA sends astronauts to Mars.
Image Credit: NASA/Isaac Watson
#SolarSystemandBeyond #NASAMarshall #jpl #psyche #asteroid
NASA’s Perseverance rover is well into its second science campaign, collecting rock-core samples from features within an area long considered by scientists to be a top prospect for finding signs of ancient microbial life on Mars. The rover has collected four samples from an ancient river delta in the Red Planet’s Jezero Crater since July 7, bringing the total count of scientifically compelling rock samples to 12.
Twenty-eight miles (45 kilometers) wide, Jezero Crater hosts a delta – an ancient fan-shaped feature that formed about 3.5 billion years ago at the convergence of a Martian river and a lake. Perseverance is currently investigating the delta’s sedimentary rocks, formed when particles of various sizes settled in the once-watery environment. During its first science campaign, the rover explored the crater’s floor, finding igneous rock, which forms deep underground from magma or during volcanic activity at the surface.
In this image, NASA’s Perseverance rover puts its robotic arm to work around a rocky outcrop called “Skinner Ridge” in Mars’ Jezero Crater. Composed of multiple images, this mosaic shows layered sedimentary rocks in the face of a cliff in the delta, as well as one of the locations where the rover abraded a circular patch to analyze a rock’s composition.
Image Credit: NASA/JPL-Caltech/ASU/MSSS
#NASAMarshall #NASAJPL #SolarSystemandBeyond #Mars #planet #Perseverance
At around 60 million light-years from Earth, the Great Barred Spiral Galaxy, NGC 1365, is captured beautifully in this image by the NASA/ESA Hubble Space Telescope. Located in the constellation of Fornax (the Furnace), the blue and fiery orange swirls show us where stars have just formed and the dusty sites of future stellar nurseries.
At the outer edges of the image, enormous star-forming regions within NGC 1365 can be seen. The bright, light-blue regions indicate the presence of hundreds of baby stars that formed from coalescing gas and dust within the galaxy's outer arms.
This Hubble image was captured as part of a joint survey with the Atacama Large Millimeter/submillimeter Array (ALMA) in Chile. The survey will help scientists understand how the diversity of galaxy environments observed in the nearby universe, including NGC 1365 and other galaxies such as NGC 2835 and NGC 2775, influence the formation of stars and star clusters. Expected to image over 100,000 gas clouds and star-forming regions beyond our Milky Way, the PHANGS survey is expected to uncover and clarify many of the links between cold gas clouds, star formation, and the overall shape and morphology of galaxies.
Image Credit: ESA/Hubble & NASA, J. Lee and the PHANGS-HST Team; Acknowledgment: Judy Schmidt (Geckzilla)
#NASA #MarshallSpaceFlightCenter #MSFC #Marshall #HubbleSpaceTelescope #HST #astronomy #space #astrophysics #solarsystemandbeyond #gsfc #Goddard #GoddardSpaceFlightCenter #ESA #EuropeanSpaceAgency #galaxy
This 2003 Chandra image of the supermassive black hole at our Galaxy's center, a.k.a. Sagittarius A* or Sgr A*, was made from the longest X-ray exposure of that region to date. In addition to Sgr A* more than two thousand other X-ray sources were detected in the region, making this one of the richest fields ever observed.
During the two-week observation period, Sgr A* flared up in X-ray intensity half a dozen or more times. The cause of these outbursts is not understood, but the rapidity with which they rise and fall indicates that they are occurring near the event horizon, or point of no return, around the black hole. Even during the flares the intensity of the X-ray emission from the vicinity of the black hole is relatively weak. This suggests that Sgr A*, weighing in at 3 million times the mass of the Sun, is a starved black hole, possibly because explosive events in the past have cleared much of the gas from around it.
Evidence for such explosions was revealed in the image - huge lobes of 20 million-degree Centigrade gas (the red loops in the image at approximately the 2 o'clock and 7 o'clock positions) that extend over dozens of light years on either side of the black hole. They indicate that enormous explosions occurred several times over the last ten thousand years.
Further analysis of the Sgr A* image is expected to give astronomers a much better understanding of how the supermassive black hole in the center of our galaxy grows and how it interacts with its environment. This knowledge will also help to understand the origin and evolution of even larger supermassive black holes found in the centers of other galaxies.
Image credit: NASA/CXC/MIT/F.K.Baganoff et al.
#NASA #MarshallSpaceFlightCenter #MSFC #Marshall #chandraxrayobservatory #ChandraXRay #cxo #chandra #astronomy #space #astrophysics #nasamarshallspaceflightcenter #solarsystemandbeyond #blackhole #supermassiveblackhole
This image shows two of Jupiter's large rotating storms, captured by Juno’s visible-light imager, JunoCam, on Juno’s 38th perijove pass, on Nov. 29, 2021.
This image was acquired at 50 degrees 5 minutes north latitude, at an altitude of 3,815 miles (6,140 kilometers). Atmospheric details as small as 2.5 miles (4 kilometers) can be discerned in the image. Bright “pop-up” clouds are visible above the lower storm, casting shadows on the cloud bank below. Although the pop-up clouds appear small in comparison to the large storm below, such clouds are typically 31 miles (50 kilometers) across.
Citizen scientist Kevin M. Gill processed the image to enhance the color and contrast, using raw JunoCam data
JunoCam's raw images are available for the public to peruse and process into image products at missionjuno.swri.edu/junocam/processing. More information about NASA citizen science can be found at science.nasa.gov/citizenscience and www.nasa.gov/solve/opportunities/citizenscience.
Image credit: NASA/JPL-Caltech/SwRI/MSSS; Image processing: Kevin M. Gill CC BY--
#NASA #MarshallSpaceFlightCenter #MSFC #Marshall #jpl #jetpropulsionlaboratory #nasamarshall #MSFC #solarsystem #juno #jupiter #space #astronomy #nasajuno #nasamarshallspaceflightcenter
NASA’s Juno spacecraft captured this view of Jupiter during the mission’s 40th close pass by the giant planet on Feb. 25, 2022. The large, dark shadow on the left side of the image was cast by Jupiter’s moon Ganymede.
Citizen scientist Thomas Thomopoulos created this enhanced-color image using raw data from the JunoCam instrument (Figure A). At the time the raw image was taken, the Juno spacecraft was about 44,000 miles (71,000 kilometers) above Jupiter’s cloud tops, at a latitude of about 55 degrees south, and 15 times closer than Ganymede, which orbits about 666,000 miles (1.1 million kilometers) away from Jupiter.
An observer at Jupiter’s cloud tops within the oval shadow would experience a total eclipse of the Sun. Total eclipses are more common on Jupiter than Earth for several reasons. Jupiter has four major moons (Galilean satellites) that often pass between Jupiter and the Sun: in seven days, Ganymede transits once; Europa, twice; and Io, four times. And since Jupiter’s moons orbit in a plane close to Jupiter’s orbital plane, the moon shadows are often cast upon the planet.
Image credit: NASA/JPL-Caltech/SwRI/MSSS Image processing by Thomas Thomopoulos © CC BY--
#NASAMarshall #nasajuno #jupiter #ganymede
Spring doesn't just hapen on Earth. Spring also happens on some of our neighboring planets in the solar system.
Of the countless equinoxes Saturn has seen since the birth of the solar system, this one, captured here in a mosaic of light and dark, is the first witnessed up close by an emissary from Earth … none other than our faithful robotic explorer, Cassini in this image from 2009.
Seen from our planet, the view of Saturn's rings during equinox is extremely foreshortened and limited. But in orbit around Saturn, Cassini had no such problems. From 20 degrees above the ring plane, Cassini's wide angle camera shot 75 exposures in succession for this mosaic showing Saturn, its rings, and a few of its moons a day and a half after exact Saturn equinox, when the sun's disk was exactly overhead at the planet's equator.
At equinox, the shadows of the planet's expansive rings are compressed into a single, narrow band cast onto the planet as seen in this mosaic. At this time so close to equinox, illumination of the rings by sunlight reflected off the planet vastly dominates any meager sunlight falling on the rings. Hence, the half of the rings on the left illuminated by planetshine is, before processing, much brighter than the half of the rings on the right. On the right, it is only the vertically extended parts of the rings that catch any substantial sunlight.
Image Credit: NASA/JPL/Space Science Institute
#NASA #Cassini #JPL #JetPropulsionLaboratory #NASAMarshall #SolarSystemandBeyond #space #astronomy #Saturn #astronomy #planet
On Earth, amethysts can form when gas bubbles in lava cool under the right conditions. In space, a dying star with a mass similar to the Sun is capable of producing a structure on par with the appeal of these beautiful gems.
As stars like the Sun run through their fuel, they cast off their outer layers and the core of the star shrinks. Using NASA’s Chandra X-ray Observatory, astronomers have found a bubble of ultra-hot gas at the center of one of these expiring stars, a planetary nebula in our galaxy called IC 4593. At a distance of about 7,800 light years from Earth, IC 4593 is the most distant planetary nebula yet detected with Chandra.
This new image of IC 4593 has X-rays from Chandra in purple, invoking similarities to amethysts found in geodes around the globe. The bubble detected by Chandra is from gas that has been heated to over a million degrees. These high temperatures were likely generated by material that blew away from the shrunken core of the star and crashed into gas that had previously been ejected by the star.
Image credit: X-ray: NASA/CXC/UNAM/J. Toalá et al.; Optical: NASA/STScI
#NASA #MarshallSpaceFlightCenter #MSFC #Marshall #chandraxrayobservatory #ChandraXRay #cxo #chandra #astronomy #space #astrophysics #nasamarshallspaceflightcenter #solarsystemandbeyond #nebula #planetarynebula #HubbleSpaceTelescope #HST #Goddard #GoddardSpaceFlightCenter #STScI
Cyclones at the north pole of Jupiter appear as swirls of striking colors in this extreme false color rendering of an image from NASA’s Juno mission. The huge, persistent cyclone found at Jupiter’s north pole is visible at the center of the image, encircled by smaller cyclones that range in size from 2,500 to 2,900 miles (4,000 to 4,600 kilometers). Together, this pattern of storms covers an area that would dwarf the Earth.
The color choices in this image reveal both the beauty of Jupiter and the subtle details present in Jupiter’s dynamic cloud structure. Each new observation that Juno provides of Jupiter’s atmosphere complements computer simulations and helps further refine our understanding of how the storms evolve over time.
The Juno mission provided the first clear views of Jupiter’s polar regions. Juno’s Jovian InfraRed Auroral Mapper (JIRAM) instrument has also mapped this area, as well as a similar pattern of storms at the planet’s south pole.
Citizen scientist Gerald Eichstädt made this composite image using data obtained by the JunoCam instrument during four of the Juno spacecraft’s close passes by Jupiter, which took place between Feb. 17, 2020, and July 25, 2020. The greatly exaggerated color is partially a result of combining many individual images to create this view.
Image Credit: Image data: NASA/JPL-Caltech/SwRI/MSSS; Image processing by Gerald Eichstädt
#NASA #MarshallSpaceFlightCenter #MSFC #Marshall #jpl #jetpropulsionlaboratory #nasamarshall #MSFC #solarsystem #juno #jupiter #space #astronomy #nasajuno #nasamarshallspaceflightcenter
During its 36th low pass over Jupiter, NASA’s Juno spacecraft captured this view of striking cloud bands and swirls in the giant planet’s mid-southern latitudes. The dark, circular vortex near the center of the image is a cyclone that spans roughly 250 miles (about 400 kilometers). The color at its center is likely to be the result of descending winds that cleared out upper-level clouds, revealing darker material below.
Citizen scientist Brian Swift used a raw JunoCam image digitally projected onto a sphere to create this view. It has been rotated so that north is up. The original image was taken on Sept. 2, 2021, at 4:09 p.m. PDT (7:09 p.m. EDT). At the time, the spacecraft was about 16,800 miles (about 27,000 kilometers) above Jupiter’s cloud tops, at a latitude of about 31 degrees south.
JunoCam's raw images are available for the public to peruse and process into image products at missionjuno.swri.edu/junocam/processing. More information about NASA citizen science can be found a science.nasa.gov/citizenscience and www.nasa.gov/solve/opportunities/citizenscience.
More information about Juno is at www.nasa.gov/juno and missionjuno.swri.edu/. For more about this finding and other science results, see www.missionjuno.swri.edu/science-findings/.
Image credit: NASA/JPL-Caltech/SwRI/MSSS; Image processing by Brian Swift © CC BY--
#NASA #MarshallSpaceFlightCenter #MSFC #Marshall #jpl #jetpropulsionlaboratory #nasamarshall #MSFC #solarsystem #juno #jupiter #space #astronomy #nasajuno #nasamarshallspaceflightcenter
2006 images from three of NASA's Great Observatories were combined to create this spectacular, multiwavelength view of the starburst galaxy M82. Optical light from stars (yellow-green/Hubble Space Telescope) shows the disk of a modest-sized, apparently normal galaxy.
Another Hubble observation designed to image 10,000 degree Celsius hydrogen gas (orange) reveals a startlingly different picture of matter blasting out of the galaxy. The Spitzer Space Telescope infrared image (red) shows that cool gas and dust are also being ejected. Chandra's X-ray image (blue) reveals gas that has been heated to millions of degrees by the violent outflow. The eruption can be traced back to the central regions of the galaxy where stars are forming at a furious rate, some 10 times faster than in the Milky Way Galaxy.
Many of these newly formed stars are very massive and race through their evolution to explode as supernovas. Vigorous mass loss from these stars before they explode, and the heat generated by the supernovas drive the gas out of the galaxy at millions of miles per hour. It is thought that the expulsion of matter from a galaxy during bursts of star formation is one of the main ways of spreading elements like carbon and oxygen throughout the universe.
The burst of star formation in M82 is thought to have been initiated by shock waves generated in a close encounter with a large nearby galaxy, M81, about 100 million years ago. These shock waves triggered the collapse of giant clouds of dust and gas in M82. In another 100 million years or so, most of the gas and dust will have been used to form stars, or blown out of the galaxy, so the starburst will subside.
Image credit: X-ray: NASA/CXC/JHU/D.Strickland; Optical: NASA/ESA/STScI/AURA/The Hubble Heritage Team; IR: NASA/JPL-Caltech/Univ. of AZ/C. Engelbracht
#NASA #MarshallSpaceFlightCenter #MSFC #Marshall #ChandraXrayObservatory #cxo #HubbleSpaceTelescope #HST #astronomy #space #astrophysics #solarsystemandbeyond #gsfc #Goddard #GoddardSpaceFlightCenter #ESA #EuropeanSpaceAgency #SpitzerSpaceTelescope #JPL #JetPropulsionLaboratory #galaxy #starburstgalaxy
Have you ever had stars in your eyes? It appears that the eye on the left does, and moreover it appears to be gazing at even more stars. The featured 27-frame mosaic was taken last July from Ojas de Salar in the Atacama Desert of Chile. The eye is actually a small lagoon captured reflecting the dark night sky as the Milky Way Galaxy arched overhead. The seemingly smooth band of the Milky Way is really composed of billions of stars, but decorated with filaments of light-absorbing dust and red-glowing nebulas. Additionally, both Jupiter (slightly left the galactic arch) and Saturn (slightly to the right) are visible. The lights of small towns dot the unusual vertical horizon. The rocky terrain around the lagoon appears to some more like the surface of Mars than our Earth.
CREDITS: Miguel Claro (TWAN, Dark Sky Alqueva)
#NASA #MarshallSpaceFlightCenter #MSFC #Marshall #milkyway #astronomy
#Saturn #Jupiter #solarsystemandbeyond #nasamarshallspaceflightcenter
The gas giant orbiter has flown over 510 million miles and also documented close encounters with three of Jupiter’s four largest moons.
NASA’s Juno spacecraft will fly past Jupiter’s volcanic moon Io on Tuesday, May 16, and then the gas giant itself soon after. The flyby of the Jovian moon will be the closest to date, at an altitude of about 22,060 miles (35,500 kilometers). Now in the third year of its extended mission to investigate the interior of Jupiter, the solar-powered spacecraft will also explore the ring system where some of the gas giant’s inner moons reside.
To date, Juno has performed 50 flybys of Jupiter and also collected data during close encounters with three of the four Galilean moons – the icy worlds Europa and Ganymede, and fiery Io.
This JunoCam image of the Jovian moon Io was collected during Juno’s flyby of the moon on March 1, 2023. At the time of closest approach, Juno was about 32,000 miles (51,500 kilometers) away from Io.
Image credit: NASA/JPL-Caltech/SwRI/MSSS Image processing: Kevin M. Gill (CC BY)
#NASA #MarshallSpaceFlightCenter #MSFC #Marshall #jpl #nasamarshall #juno #nasajuno #Io
As NASA’s Juno mission completed its 43rd close flyby of Jupiter on July 5, 2022, its JunoCam instrument captured this striking view of vortices — hurricane-like spiral wind patterns — near the planet’s north pole.
These powerful storms can be over 30 miles (50 kilometers) in height and hundreds of miles across. Figuring out how they form is key to understanding Jupiter's atmosphere, as well as the fluid dynamics and cloud chemistry that create the planet’s other atmospheric features. Scientists are particularly interested in the vortices’ varying shapes, sizes, and colors. For example, cyclones, which spin counter-clockwise in the northern hemisphere and clockwise in the southern, and anti-cyclones, which rotate clockwise in the northern hemisphere and counter-clockwise in the southern hemisphere, exhibit very different colors and shapes.
A NASA citizen science project, Jovian Vortex Hunter, seeks help from volunteer members of the public to spot and help categorize vortices and other atmospheric phenomena visible in JunoCam photos of Jupiter. This process does not require specialized training or software, and can be done by anyone, anywhere, with a cellphone or laptop. As of July 2022, 2,404 volunteers had made 376,725 classifications using the Jovian Vortex Hunter project web site at www.zooniverse.org/projects/ramanakumars/jovian-vortex-hu....
Another citizen scientist, Brian Swift, created this enhanced color and contrast view of vortices using raw JunoCam image data. At the time the raw image was taken, the Juno spacecraft was about 15,600 miles (25,100 kilometers) above Jupiter’s cloud tops, at a latitude of about 84 degrees.
JunoCam's raw images are available for the public to peruse and process into image products at missionjuno.swri.edu/junocam/processing. More information about NASA citizen science can be found at science.nasa.gov/citizenscience and www.nasa.gov/solve/opportunities/citizenscience.
More information about Juno is at www.nasa.gov/juno and missionjuno.swri.edu. For more about this finding and other science results, see www.missionjuno.swri.edu/science-findings.
Image data: NASA/JPL-Caltech/SwRI/MSSS; Image processing by Brian Swift © CC BY
#NASA #MarshallSpaceFlightCenter #MSFC #Marshall #jpl #jetpropulsionlaboratory #nasamarshall #juno ter #nasajuno
JunoCam took this image of Jupiter’s northernmost cyclone (visible to the right along the bottom edge of image) on Sept. 29, 2022.
Image credit: NASA/JPL-Caltech/SwRI/MSSS Image processing: Navaneeth Krishnan S CC BY 3.0
#NASA #MarshallSpaceFlightCenter #MSFC #Marshall #jpl #jetpropulsionlaboratory #nasamarshall #juno #nasajuno #Io
The Helix Nebula is an example of a planetary nebula. Though it looks like a bubble or eye from Earth’s point of view, the Helix is actually a trillion-mile-long tunnel of glowing gases. In its center lies a white dwarf star.
Image credit: NASA, NOAO, ESA, the Hubble Helix Nebula Team, M. Meixner (STScI), and T.A. Rector (NRAO)
#NASA #MarshallSpaceFlightCenter #MSFC #Marshall #HubbleSpaceTelescope #HST #astronomy #space #astrophysics #solarsystemandbeyond #gsfc #Goddard #GoddardSpaceFlightCenter #ESA #EuropeanSpaceAgency #nebula #planetarynebula
The first picture NASA's Juno spacecraft took as it flew by Jupiter's ice-encrusted moon Europa has arrived on Earth. Revealing surface features in a region near the moon's equator called Annwn Regio, the image was captured during the solar-powered spacecraft's closest approach, on Thursday, Sept. 29, at 2:36 a.m. PDT (5:36 a.m. EDT), at a distance of about 219 miles (352 kilometers).
Image data: NASA/JPL-Caltech/SWRI/MSSS
#NASA #MarshallSpaceFlightCenter #MSFC #Marshall #jpl #jetpropulsionlaboratory #nasamarshall #juno #nasajuno #europa
What are those dots between Saturn's rings? Our Earth and Moon. Just over three years ago, because the Sun was temporarily blocked by the body of Saturn, the robotic Cassini spacecraft was able to look toward the inner Solar System. There, it spotted our Earth and Moon -- just pin-pricks of light lying about 1.4 billion kilometers distant. Toward the right of the featured image is Saturn's A ring, with the broad Encke Gap on the far right and the narrower Keeler Gap toward the center. On the far left is Saturn's continually changing F Ring. From this perspective, the light seen from Saturn's rings was scattered mostly forward , and so appeared backlit. After more than a decade of exploration and discovery, the Cassini spacecraft ran low on fuel in 2017 and was directed to enter Saturn's atmosphere, where it surely melted.
Image Credit: NASA, ESA, JPL-Caltech, SSI, Cassini Imaging Team; Processing & License: Kevin M. Gill
Phosphorus, a key chemical element for many biological processes, has been found in icy grains emitted by the small moon and is likely abundant in its subsurface ocean.
Using data collected by NASA’s Cassini mission, an international team of scientists has discovered phosphorus – an essential chemical element for life – locked inside salt-rich ice grains ejected into space from Enceladus.
The small moon is known to possess a subsurface ocean, and water from that ocean erupts through cracks in Enceladus' icy crust as geysers at its south pole, creating a plume. The plume then feeds Saturn's E ring (a faint ring outside of the brighter main rings) with icy particles.
During its mission at the gas giant from 2004 to 2017, Cassini flew through the plume and E ring numerous times. Scientists found that Enceladus' ice grains contain a rich array of minerals and organic compounds – including the ingredients for amino acids – associated with life as we know it.
In this image, seen as a bright arc in this 2006 observation by Cassini, Saturn’s E ring is fed with icy particles from Enceladus’ plume, creating wispy fingers of bright material that is backlit by the Sun. The shadowed hemisphere of the moon can be seen as a dark dot inside the ring.
Image Credit: NASA/JPL-Caltech/Space Science Institute
#NASA #Cassini #JPL #JetPropulsionLaboratory #NASAMarshall #SolarSystemandBeyond #space #astronomy #Saturn #astronomy #planet #Enceladus
This 2016 image of haze layers above Pluto’s limb was taken by the Ralph/Multispectral Visible Imaging Camera (MVIC) on NASA’s New Horizons spacecraft. About 20 haze layers are seen; the layers have been found to typically extend horizontally over hundreds of kilometers, but are not strictly parallel to the surface. For example, scientists note a haze layer about 3 miles (5 kilometers) above the surface (lower left area of the image), which descends to the surface at the right.
Image Credit: NASA/JHUAPL/SwRI
#NASA #NASAMarshall #NASAMarshallSpaceFlightCenter #MSFC #NewHorizons #SolarSystemandBeyond #Pluto #AmesResearchCenter #ARC #marshallspaceflightcenter #NewFrontiers #gsfc #Goddard #GoddardSpaceFlightCenter #JPL #JetPropulsionLaboratory
Chandra's image of the elliptical galaxy NGC 4697 reveals diffuse hot gas dotted with many point-like sources. As in the elliptical galaxies, NGC 4649 and NGC 1553, the point-like sources are due to black holes and neutron stars in binary star systems. Material pulled off a normal star is heated and emits X-radiation as it falls toward its black hole or neutron star companion.
Black holes and neutron stars are the end state of the brightest and most massive stars. Chandra's detection of numerous neutron stars and black holes in this and other elliptical galaxies shows that these galaxies once contained many very bright, massive stars, in marked contrast to the present population of low-mass faint stars that now dominate elliptical galaxies.
An unusually large number of the binary star X-ray sources in NGC 4697 are in "globular star clusters," round balls of stars in the galaxy that contain about one million stars in a volume where typically only one would be found. This suggests that the extraordinarily dense environment of globular clusters may be a good place for black holes or neutron stars to capture a companion star.
The origin of the hot gas cloud enveloping the galaxy is not known. One possibility is that the gas lost by evaporation from normal stars- so-called stellar winds - is heated by these winds and by supernova explosions.
Image credit: NASA/CXC/UVa/C.Sarazin et al.
#NASA #MarshallSpaceFlightCenter #MSFC #Marshall #chandraxrayobservatory #ChandraXRay #cxo #chandra #astronomy #space #astrophysics #nasamarshallspaceflightcenter #solarsystemandbeyond #galaxy #blackhole #neutronstar
The Orion Nebula is a picture book of star formation, from the massive, young stars shaping the nebula to the pillars of dense gas that may be the homes of budding stars. The Trapezium resides in the bright central region. Ultraviolet light unleashed by these stars carves a cavity in the emission nebula and disrupts the growth of hundreds of smaller stars.
Image credit: NASA,ESA, M. Robberto (STScI/ESA) and the Hubble Space Telescope Orion Treasury Project Team
#NASA #MarshallSpaceFlightCenter #MSFC #Marshall #HubbleSpaceTelescope #HST #astronomy #space #astrophysics #solarsystemandbeyond #gsfc #Goddard #GoddardSpaceFlightCenter #ESA #EuropeanSpaceAgency #nebula #nebula
The interaction of two doomed stars has created this spectacular ring adorned with bright clumps of gas -– a diamond necklace of cosmic proportions. Fittingly known as the “Necklace Nebula,” this planetary nebula is located 15,000 light-years away from Earth in the small, dim constellation of Sagitta (the Arrow).
A pair of tightly orbiting Sun-like stars produced the Necklace Nebula, which also goes by the less glamorous name of PN G054.203.4. Roughly 10,000 years ago, one of the aging stars expanded and engulfed its smaller companion, creating something astronomers call a “common envelope.” The smaller star continued to orbit inside its larger companion, increasing the bloated giant’s rotation rate until large parts of it spun outwards into space. This escaping ring of debris formed the Necklace Nebula, with particularly dense clumps of gas forming the bright “diamonds” around the ring.
The pair of stars which created the Necklace Nebula remain so close together – separated by only several million miles – that they appear as a single bright dot in the center of this image. Despite their close encounter, the stars are still furiously whirling around each other, completing an orbit in just over a day.
Image credit: ESA/Hubble & NASA, K. Noll
#NASA #MarshallSpaceFlightCenter #MSFC #Marshall #HubbleSpaceTelescope #HST #astronomy #space #astrophysics #solarsystemandbeyond #gsfc #Goddard #GoddardSpaceFlightCenter #ESA #EuropeanSpaceAgency
Though Mars is the Red Planet, false-color images can help us learn about its weather and geology. This image shows a variety of wind-related features on the Red Planet near the center of Gamboa Crater. Larger sand dunes form sinuous crests and individual domes.
There are tiny ripples on the tops of the dunes, only several feet from crest-to-crest. These merge into larger mega-ripples about 30 feet apart that radiate outward from the dunes. The larger, brighter formations that are roughly parallel are called "Transverse Aeolian Ridges" (TAR). These TAR are covered with very coarse sand.
The mega-ripples appear blue-green on one side of an enhanced color cutout while the TAR appear brighter blue on the other. This could be because the TAR are actively moving under the force of the wind, clearing away darker dust and making them brighter. All of these different features can indicate which way the wind was blowing when they formed. Being able to study such variety so close together allows us to see their relationships and compare and contrast features to examine what they are made of and how they formed.
Image Credit: NASA/JPL-Caltech/University of Arizona
#NASA #jpl #jetpropulsionlaboratory #marshallspaceflightcenter #msfc #mars #moontomars #planet #space #MarsReconnaissanceOrbiter #MRO
Centaurus A sports a warped central disk of gas and dust, which is evidence of a past collision and merger with another galaxy. It also has an active galactic nucleus that periodically emits jets. It is the fifth brightest galaxy in the sky and only about 13 million light-years away from Earth, making it an ideal target to study an active galactic nucleus – a supermassive black hole emitting jets and winds – with NASA's upcoming James Webb Space Telescope.
Image credit: NASA/CXC/C.Lisse & S.Wolk
#NASA #MarshallSpaceFlightCenter #MSFC #Marshall #chandraxrayobservatory #ChandraXRay #cxo #chandra #astronomy #space #astrophysics #nasamarshallspaceflightcenter #solarsystemandbeyond #comet
This image from NASA’s Juno mission captures the northern hemisphere of Jupiter around the region known as Jet N7. The planet’s strong winds create the many swirling storms visible near the top of its atmosphere. Data from Juno helped scientists discover another, less visible effect of those winds: Jupiter’s powerful magnetic field changes over time. The winds extend more than 1800 miles (3000 kilometers) deep, where the material lower in Jupiter’s atmosphere is highly conductive, electrically. Scientists determined that the wind shears this conductive material apart and carries it around the planet, which changes the shape of the magnetic field.
Citizen scientist Kevin M. Gill created this false-color image using data from the JunoCam camera. The original image was taken on February 21, 2021 as the Juno spacecraft performed its 32nd close flyby of Jupiter. At the time, the spacecraft was about 10,200 miles (16,400 kilometers) from the tops of the clouds at a latitude of about 66 degrees north.
Image Credit: Image data: NASA/JPL-Caltech/SwRI/MSSS; Image processing by Kevin M. Gill © CC BY
#NASA #MarshallSpaceFlightCenter #MSFC #Marshall #jpl #jetpropulsionlaboratory #nasamarshall #MSFC #solarsystem #juno #jupiter #space #astronomy #nasajuno #nasamarshallspaceflightcenter #GreatRedSpot
Signs of a planet transiting a star outside of the Milky Way galaxy may have been detected for the first time. This intriguing result, using NASA’s Chandra X-ray Observatory, opens up a new window to search for exoplanets at greater distances than ever before.
The possible exoplanet candidate is located in the spiral galaxy Messier 51 (M51), also called the Whirlpool Galaxy because of its distinctive profile.
Exoplanets are defined as planets outside of our Solar System. Until now, astronomers have found all other known exoplanets and exoplanet candidates in the Milky Way galaxy, almost all of them less than about 3,000 light-years from Earth. An exoplanet in M51 would be about 28 million light-years away, meaning it would be thousands of times farther away than those in the Milky Way.
This composite image of M51 with X-rays from Chandra and optical light from NASA's Hubble Space Telescope contains a box that marks the location of the possible planet candidate.
Image credit: X-ray: NASA/CXC/SAO/R. DiStefano, et al.; Optical: NASA/ESA/STScI/Grendler
#NASA #MarshallSpaceFlightCenter #MSFC #Marshall #ChandraXrayObservatory #cxo #HubbleSpaceTelescope #HST #astronomy #space #astrophysics #solarsystemandbeyond #gsfc #Goddard #GoddardSpaceFlightCenter #ESA #EuropeanSpaceAgency #galaxy
A multitude of magnificent, swirling clouds in Jupiter's dynamic North North Temperate Belt is captured in this image from NASA's Juno spacecraft. Appearing in the scene are several bright-white "pop-up" clouds as well as an anticyclonic storm, known as a white oval.
This color-enhanced image was taken at 4:58 p.m. EDT on Oct. 29, 2018 as the spacecraft performed its 16th close flyby of Jupiter. At the time, Juno was about 4,400 miles from the planet's cloud tops, at a latitude of approximately 40 degrees north.
Citizen scientists Gerald Eichstädt and Seán Doran created this image using data from the spacecraft's JunoCam imager
Image Credit: Enhanced Image by Gerald Eichstädt and Sean Doran (CC BY-NC-SA)/NASA/JPL-Caltech/SwRI/MSSS
NGC 4666 takes center stage in this image from the NASA/ESA Hubble Space Telescope. This majestic spiral galaxy lies about 80 million light-years away in the constellation Virgo and is undergoing a particularly intense episode of star formation. Astronomers refer to galaxies that rapidly form stars as starburst galaxies. NGC 4666’s starburst is likely due to gravitational interactions with its unruly neighbors – including the nearby galaxy NGC 4668 and a dwarf galaxy, which is a small galaxy made up of a few billion stars.
NGC 4666’s burst of star formation is driving an unusual form of extreme galactic weather known as a superwind – a gigantic transfer of gas from the bright central heart of the galaxy out into space. This superwind is the result of driving winds from short-lived massive stars formed during NGC 4666’s starburst as well as spectacularly energetic supernova explosions. Two supernovae occurred in NGC 4666 within the last decade – one in 2014 and the other in 2019. The star that led to the 2019 supernova was 19 times as massive as our Sun!
Though the torrent of superheated gas emanating from NGC 4666 is truly vast in scale – extending for tens of thousands of light-years – it is invisible in this image. The superwind’s extremely high temperature makes it stand out as a luminous plume in X-ray or radio observations, but it doesn’t show up at the visible wavelengths imaged by Hubble’s Wide Field Camera 3.
Image credit: ESA/Hubble & NASA, O. Graur; Acknowledgment: L. Shatz
#NASA #MarshallSpaceFlightCenter #MSFC #Marshall #HubbleSpaceTelescope #HST #astronomy #space #astrophysics #solarsystemandbeyond #gsfc #Goddard #GoddardSpaceFlightCenter #ESA #EuropeanSpaceAgency #galaxy
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.
Image Credit: NASA, ESA and Jesús Maíz Apellániz (IAA, Spain); Acknowledgement: Davide De Martin (ESA/Hubble)
#NASA #MarshallSpaceFlightCenter #MSFC #Marshall #HubbleSpaceTelescope #HST #astronomy #space #astrophysics #Goddard #GoddardSpaceFlightCenter #ESA #EuropeanSpaceAgency #galaxy #supernova #solarsystemandbeyond #gsfc #nebula #opennebula
N44 is a complex nebula filled with glowing hydrogen gas, dark lanes of dust, massive stars, and many populations of stars of different ages. One of its most distinctive features, however, is the dark, starry gap called a “superbubble,” visible in this Hubble Space Telescope image in the upper central region.
The hole is about 250 light-years wide and its presence is still something of a mystery. Stellar winds expelled by massive stars in the bubble's interior may have driven away the gas, but this is inconsistent with measured wind velocities in the bubble. Another possibility, since the nebula is filled with massive stars that would expire in titanic explosions, is that the expanding shells of old supernovae sculpted the cosmic cavern.
Astronomers have found one supernova remnant in the vicinity of the superbubble and identified an approximately 5 million year difference in age between stars within and at the rim of the superbubble, indicating multiple, chain-reaction star-forming events. The deep blue area at about 5 o’clock around the superbubble is one of the hottest regions of the nebula and the area of the most intense star formation.
N44 is an emission nebula, which means its gas has been energized, or ionized, by the radiation of nearby stars. As the ionized gas begins to cool from its higher-energy state to a lower-energy state, it emits energy in the form of light, causing the nebula to glow. Located in the Large Magellanic Cloud, N44 spans about 1,000 light-years and is about 170,000 light-years away from Earth.
Image credit: NASA, ESA, V. Ksoll and D. Gouliermis (Universität Heidelberg), et al.; Processing: Gladys Kober (NASA/Catholic University of America)
#NASA #MarshallSpaceFlightCenter #MSFC #Marshall #HubbleSpaceTelescope #HST #astronomy #space #astrophysics #solarsystemandbeyond #gsfc #Goddard #GoddardSpaceFlightCenter #ESA #EuropeanSpaceAgency #supernovaremnant #nebula #supernova
NASA’s Mars 2020 Perseverance rover performed its first drive on Mars March 4, covering 21.3 feet (6.5 meters) across the Martian landscape. The drive served as a mobility test that marks just one of many milestones as team members check out and calibrate every system, subsystem, and instrument on Perseverance. Once the rover begins pursuing its science goals, regular commutes extending 656 feet (200 meters) or more are expected.
This image was captured while NASA’s Perseverance rover drove on Mars for the first time on March 4, 2021. One of Perseverance’s Hazard Avoidance Cameras (Hazcams) captured this image as the rover completed a short traverse and turn from its landing site in Jezero Crater.
Image Credit: NASA/JPL-Caltech
#NASA #jpl #jetpropulsionlaboratory #marshallspaceflightcenter #msfc #mars #moontomars #planet #space #CountdownToMars