Suggested Searches

Chandra X-ray Observatory

The guitar shape in the “Guitar Nebula” comes from bubbles blown by particles ejected from the pulsar through a steady...
The guitar shape in the “Guitar Nebula” comes from bubbles blown by particles ejected from the pulsar through a steady...
The guitar shape in the “Guitar Nebula” comes from bubbles blown by particles ejected from the pulsar through a steady wind as it moves through space. Images from Chandra taken in 2000, 2006, 2012 and 2021 have been combined with a single image in optical light from Palomar. X-rays from Chandra show a filament of energetic matter and antimatter particles, about two light-years long, blasting away from the pulsar (seen as the bright white dot). The movie shows how this filament has changed over two decades. An inset shows a closeup of the “guitar head” from NASA’s Hubble Space Telescope also changing over time from 1994-2021.
The guitar shape in the “Guitar Nebula” comes from bubbles blown by particles ejected from the pulsar through a steady...
The guitar shape in the “Guitar Nebula” comes from bubbles blown by particles ejected from the pulsar through a steady...
The guitar shape in the “Guitar Nebula” comes from bubbles blown by particles ejected from the pulsar through a steady wind as it moves through space. Images from Chandra taken in 2000, 2006, 2012 and 2021 have been combined with a single image in optical light from Palomar. X-rays from Chandra show a filament of energetic matter and antimatter particles, about two light-years long, blasting away from the pulsar (seen as the bright white dot). The movie shows how this filament has changed over two decades. An inset shows a closeup of the “guitar head” from NASA’s Hubble Space Telescope also changing over time from 1994-2021.
This artist’s illustration shows a red, early-Universe dwarf galaxy that hosts a rapidly feeding black hole at its center. Using...
This release features an illustration of the galaxy in which black hole LID-568 resides. A smaller illustration of black hole itself, in an outlined box, is superimposed on top of the galaxy image toward our upper right. Two lines extend from a single point in the middle of the galaxy and terminate on corners of the outlined box containing the black hole illustration. The placement of the lines and outlined box indicate that the superimposed black hole image is an enlargement of a tiny place in the center of the galaxy.
In the Cygnus OB2 star cluster, giant stars send out large amounts of high-energy radiation that can disrupt relatively fragile...
In the Cygnus OB2 star cluster, giant stars send out large amounts of high-energy radiation that can disrupt relatively fragile disks of dust and gas that are in the process of coalescing to form new planets. These images show NASA's Chandra X-ray Observatory data detailing the diffuse X-ray emission and young stars, with infrared data from NASA's Spitzer Space Telescope revealing young stars and the cooler dust and gas throughout the region. These data were used to create the best census of young stars in the cluster.
This artist's impression shows the aftermath of a supermassive black hole having destroyed a star. Tidal forces from the black...
This release features an artist's rendering that illustrates the destructive power of a supermassive black hole. The digital image depicts a disk of stellar material surrounding one such black hole. At its outer edge a neighboring star is colliding with and flying through the disk. The black hole sits halfway down our right edge of the vertical image. It resembles a jet black semicircle with a domed cap of pale blue light. The bottom half of the circular black hole is hidden behind the disk of stellar material. In this illustration, the disk is viewed edge on. It resembles a band of swirling yellow, orange, and red gas, cutting diagonally from our middle right toward our lower left. Near our lower left, the outer edge of the stellar debris disk overlaps with a bright blue sphere surrounded by luminous white swirls. This sphere represents a neighboring star crashing through the disk. The stellar disk is the wreckage of a destroyed star. An electric blue and white wave shows the hottest gas in the disk. As the neighboring star crashes through the disk it leaves behind a trail of gas depicted as streaks of fine mist. Bursts of X-rays are released and are detected by Chandra. Superimposed in the upper left corner of the illustration is an inset box showing a close up image of the source in X-ray and optical light. X-ray light is shown as purple and optical light is white and beige.
Researchers have discovered a second pair of tails trailing behind a galaxy in this cluster. Previously, astronomers discovered a shorter...
Researchers have discovered a second pair of tails trailing behind a galaxy in this cluster. Previously, astronomers discovered a shorter pair of tails from a different galaxy close to this latest one. This newer and longer set of tails was only seen because of a deeper observation with Chandra that revealed the fainter X-rays that have been shown in the optical data. These tails span for over a million light-years and help determine the evolution of the galaxy cluster.
Researchers using Chandra, Swift, and XMM-Newton data have made important headway in understanding how – and when – a supermassive...
Researchers using Chandra, Swift, and XMM-Newton data have made important headway in understanding how — and when — a supermassive black hole obtains and then consumes material. This artist’s illustration shows a star that has partially been disrupted by a giant black hole in the system known as AT2018fyk. Astronomers correctly predicted when the black hole’s last snack on the star’s debris ended and predicted its next snack would begin between May and August of 2025. As long as the star survives the disruptions, these meals should occur every 3.5 years.
Researchers took note of AT2018fyk in 2018 when the optical ground-based survey ASAS-SN detected that the system had become much...
Researchers took note of AT2018fyk in 2018 when the optical ground-based survey ASAS-SN detected that the system had become much brighter. After observing it with NASA’s NICER and Chandra, and XMM-Newton, researchers determined that the surge in brightness came from a tidal disruption event (TDE), which signals that a star was completely torn apart and partially ingested after flying too close to a black hole. In this image, Chandra data of AT2018fyk is shown as an inset of an optical image of a wider field-of-view of the area.
These images were released to commemorate the 25th anniversary of Chandra. They represent the wide range of objects that the...
This image shows a collection of 25 new space images celebrating the Chandra X-ray Observatory's 25th anniversary. The images are arranged in a grid, displayed as five images across in five separate rows. Starting from the upper left, and going across each row, the objects imaged are: Crab Nebula, Orion Nebula, The Eyes Galaxies, Cat's Paw Nebula, Milky Way's Galactic Center, M16, Bat Shadow, NGC 7469, Virgo Cluster, WR 124, G21.5-0.9, Centaurus A, Cassiopeia A, NGC 3532, NGC 6872, Hb 5, Abell 2125, NGC 3324, NGC 1365, MSH 15-52, Arp 220, Jupiter, NGC 1850, MACS J0035, SN 1987A.
The Cassiopeia A supernova remnant has been observed for more than 2 million seconds since the start of the Chandra...
This image features the Cassiopeia A supernova, an expanding ball of matter and energy ejected from an exploding star. Here, rings of neon blue and brilliant white emit veins of polished gold. The rings and their arching veins encircle a place of relative calm at the center of the supernova remnant. This hole at the center of the circle, and the three-dimensionality conveyed by the rings and their arching veins, give this image of Cassiopeia A the look of a giant, crackling, electric blue donut. X-rays detected by Chandra show debris from the destroyed star and the blast wave from the explosion.
This region of star formation contains the Pillars of Creation, which was made famous by the Hubble Space Telescope. Chandra...
This composite image features a region of star formation known as the Pillars of Creation. Here, tall columns of grey gas and dust emerge from the bottom edge of the image, stretching toward our upper right. Backed by dark orange and pink mist, the cloudy grey columns are surrounded by dozens of soft, glowing, dots in whites, reds, blues, yellows, and purples. These dots are young stars emitting X-ray and infrared light. Churning with turbulent gas and dust, the columns lean to our right with small offshoots pointing in the same direction. The misty glow, colorful stars, and lifelike grey dust formations combine to create an image of yearning cloud creatures at dusk, reaching for something just out of frame.
Cosmic Road Trip: four distinct composite images from NASA's Chandra X-ray Observatory and the James Webb Space Telescope, presented in...
Cosmic Road Trip: four distinct composite images from NASA's Chandra X-ray Observatory and the James Webb Space Telescope, presented in a two-by-two grid, Rho Ophiuchi at lower right, the heart of the Orion Nebula at upper right, the galaxy NGC 3627 at lower left and the galaxy cluster MACS J0416.
Rho Ophiuchi is a cloud complex filled with gas and stars of different sizes and ages.
Rho Ophiuchi, a cloud complex filled with gas, and dotted with stars. The murky green and gold cloud resembles a ghostly head in profile, swooping down from the upper left, trailing tendrils of hair. Cutting across the bottom edge and lower righthand corner of the image is a long, narrow, brick red cloud which resembles the ember of a stick pulled from a fire. Several large white stars dot the image. Many are surrounded by glowing neon purple rings, and gleam with diffraction spikes.
The Orion Nebula.
The young star nursery at the heart of the Orion Nebula resembles a dense, stringy, dusty rose cloud, peppered with thousands of glowing golden, white, and blue stars. Layers of cloud around the edges of the image, and a concentration of bright stars at its distant core, help convey the depth of the nebula.
Spiral galaxy NGC 3627.
The galaxy NGC 3627 appears pitched at an oblique angle, tilted from our upper left down to our lower right. Much of its face is angled toward us, making its spiral arms, composed of red and purple dots, easily identifiable. Several bright white dots ringed with neon purple speckle the galaxy. At the galaxy’s core, where the spiral arms converge, a large white and purple glow identified by Chandra provides evidence of a supermassive black hole.
ACS J0416 galaxy cluster.
Here is the distant galaxy cluster known as MACS J0416. The blackness of space is packed with glowing dots and tiny shapes, in whites, purples, oranges, golds, and reds, each a distinct galaxy. Upon close inspection (and with a great deal of zooming in!) the spiraling arms of some of the seemingly tiny galaxies are revealed in this highly detailed image. Gently arched across the middle of the frame is a soft band of purple; a reservoir of superheated gas detected by Chandra.
Star Cluster Westerlund 1.
Star Cluster Westerlund 1.
Abell 478 and NGC 5044.
Abell 478 and NGC 5044.
Abell 478 and NGC 5044 (Labeled)
Abell 478 and NGC 5044 (Labeled)
Wide Field Views of Abell 478 [Left] and NGC 5044 [Right].
Wide Field Views of Abell 478 [Left] and NGC 5044 [Right].
Chandra data reveal several X-ray ridges that astronomers think are the walls of a tunnel, shaped like a cylinder, which...
This image shows a region near the center of our Milky Way galaxy in X-ray and radio light. At the bottom of the image, near the center, is a brilliant, tangled knot of material that resembles a paint splatter. This is the brightest region in the image, and it contains the supermassive black hole at center of our galaxy, known as Sagittarius A*. Rising up from Sagittarius A* in the center of the image is a pillar of blue light referred to as a chimney. This chimney of hot gas is surrounded by red clouds that are filled with stars, presenting themselves as tiny red flecks. Near the top of the blue pillar is a streak of light blue, outlined by an illustrated, gray box. This streak is referred to as the chimney exhaust vent. Just to our left is another illustrated box that shows the close-up image of the chimney vent as observed by Chandra.
Supernova Remnant SNR 1181
Supernova Remnant SNR 1181
Quasar H1821+643.
Quasar H1821+643.
Galaxy cluster SDSS J1531+3414
Galaxy cluster SDSS J1531+3414
Multiwavelength Image of SDSS J1531, Labeled
Multiwavelength Image of SDSS J1531, Labeled
Cold and warm gas located near the opening of the cavity.
Cold and warm gas located near the opening of the cavity.
This artist's illustration shows a cross-section of the supermassive black hole and surrounding material in the center of our galaxy....
This artist's illustration shows a cross-section of the supermassive black hole and surrounding material in the center of our galaxy.
Data from Chandra and Webb of the supernova remnant Cassiopeia A (Cas A) have been combined for the first time,...
Data from Chandra and Webb of the supernova remnant Cassiopeia A (Cas A) have been combined for the first time, helping to explain an unusual structure within the debris field and address other questions about the supernova explosion that created it. These images show X-rays from Chandra, infrared data from Webb and Spitzer, and optical data from Hubble. Astronomers using these data found that the so-called Green Monster near the center of Cas A was created by a blast wave from the exploded star slamming into material surrounding it.
Data from Chandra and Webb of the supernova remnant Cassiopeia A (Cas A) have been combined for the first time,...
Data from Chandra and Webb of the supernova remnant Cassiopeia A (Cas A) have been combined for the first time, helping to explain an unusual structure within the debris field and address other questions about the supernova explosion that created it. These images show X-rays from Chandra, infrared data from Webb and Spitzer, and optical data from Hubble. Astronomers using these data found that the so-called Green Monster near the center of Cas A was created by a blast wave from the exploded star slamming into material surrounding it.
This deep dataset from Chandra of the remains of a supernova known as 30 Doradus B (30 Dor B) reveals...
This deep dataset from Chandra of the remains of a supernova known as 30 Doradus B (30 Dor B) reveals evidence for more than one supernova explosion in the history of this remnant. Unusual structures in the Chandra data cannot be explained by a single explosion. These images of 30 Dor B also show optical data from the Blanco telescope in Chile, and infrared data from Spitzer. Additional data from Hubble highlights sharp features in the image.
This composite image shows the Christmas Tree Cluster. The blue and white lights (which blink in the animated version of...
This composite image shows the Christmas Tree Cluster. The blue and white lights (which blink in the animated version of this image) are young stars that give off X-rays detected by NASA’s Chandra X-ray Observatory. Optical data from the National Science Foundation’s WIYN 0.9-meter telescope on Kitt Peak shows gas in the nebula in green, corresponding to the “pine needles” of the tree, and infrared data from the Two Micron All Sky Survey shows foreground and background stars in white. This image has been rotated clockwise by about 160 degrees from the astronomer’s standard of North pointing upward, so that it appears like the top of the tree is toward the top of the image.
This composite image shows the Christmas Tree Cluster. The blue and white lights (which blink in the animated version of...
A cluster brimming with millions of stars glistens like an iridescent opal in this image from NASA's Spitzer Space Telescope....
A cluster brimming with millions of stars glistens like an iridescent opal in this image from NASA's Spitzer Space Telescope. Called Omega Centauri, the sparkling orb of stars is like a miniature galaxy. It is the biggest and brightest of the 150 or so similar objects, called globular clusters, that orbit around the outside of our Milky Way galaxy. Stargazers at southern latitudes can spot the stellar gem with the naked eye in the constellation Centaurus. Globular clusters are some of the oldest objects in our universe. Their stars are over 12 billion years old, and, in most cases, formed all at once when the universe was just a toddler. Omega Centauri is unusual in that its stars are of different ages and possess varying levels of metals, or elements heavier than boron. Astronomers say this points to a different origin for Omega Centauri than other globular clusters: they think it might be the core of a dwarf galaxy that was ripped apart and absorbed by our Milky Way long ago. In this new view of Omega Centauri, Spitzer's infrared observations have been combined with visible-light data from the National Science Foundation's Blanco 4-meter telescope at Cerro Tololo Inter-American Observatory in Chile. Visible-light data with a wavelength of .55 microns is colored blue, 3.6-micron infrared light captured by Spitzer's infrared array camera is colored green and 24-micron infrared light taken by Spitzer's multiband imaging photometer is colored red. Where green and red overlap, the color yellow appears. Thus, the yellow and red dots are stars revealed by Spitzer. These stars, called red giants, are more evolved, larger and dustier. The stars that appear blue were spotted in both visible and 3.6-micron-, or near-, infrared light. They are less evolved, like our own sun. Some of the red spots in the picture are distant galaxies beyond our own.
The Galactic Center sonification, using data from NASA’s Chandra, Hubble and Spitzer space telescopes, has been translated into a new...
The Galactic Center sonification, using data from NASA’s Chandra, Hubble and Spitzer space telescopes, has been translated into a new composition with sheet music and score. Working with a composer, this soundscape can be played by musicians.
This image contains the most distant black hole ever detected in X-rays, a result that may explain how some of...
Astronomers found the most distant black hole ever detected in X-rays (in a galaxy dubbed UHZ1) using the Chandra and Webb space telescopes. X-ray emission is a telltale signature of a growing supermassive black hole. This result may explain how some of the first supermassive black holes in the universe formed. This image shows the galaxy cluster Abell 2744 that UHZ1 is located behind, in X-rays from Chandra and infrared data from Webb, as well as close-ups of the black hole host galaxy UHZ1.
This montage features images of five different objects, ranging from a distant galaxy to a relatively close supernova remnant. Each...
Chandra Year of Light Image
The Chandra X-ray image of Hydra A, a galaxy cluster 840 million light years from Earth, shows strands of 35-40...
This image of the Hydra A galaxy cluster was taken on Oct. 30, 1999, with the Advanced CCD Imaging Spectrometer
On the left, an optical image from the Digitized Sky Survey shows Cygnus X-1, outlined in a red box. Cygnus...