Cassiopeia a supernova hi-res stock photography and images

Cassiopeia A, Cas A, Supernova Remnant Stock Photo

RMHRJ6N2–Cassiopeia A, Cas A, Supernova Remnant

The many sides of the supernova remnant Cassiopeia A. Located 10,000 light-years away in the northern constellation Cassiopeia, Cassiopeia A is the remnant of a once massive star that died in a violent supernova explosion 325 years ago. Hubble Space Telescope (HST), Spitzer Space Telescope. Stock Photo

RMD99A54–The many sides of the supernova remnant Cassiopeia A. Located 10,000 light-years away in the northern constellation Cassiopeia, Cassiopeia A is the remnant of a once massive star that died in a violent supernova explosion 325 years ago. Hubble Space Telescope (HST), Spitzer Space Telescope.

The Cassiopeia A supernova remnant is seen in a new three-dimensional format by combining data from Chandra, NASA's Spitzer Space Telescope, and ground-based facilities to construct a unique 3D model of the 300-year old remains of a stellar explosion that blew a massive star apart, sending the stellar debris rushing into space at millions of miles per hour November 15, 2013. Stock Photo

RMDHX95W–The Cassiopeia A supernova remnant is seen in a new three-dimensional format by combining data from Chandra, NASA's Spitzer Space Telescope, and ground-based facilities to construct a unique 3D model of the 300-year old remains of a stellar explosion that blew a massive star apart, sending the stellar debris rushing into space at millions of miles per hour November 15, 2013.

Composite of Cassiopeia A supernova remnant across the spectrum: Gamma rays (magenta) Fermi Gamma-ray Space Telescope; X-rays (blue, green) Chandra X-ray Observatory Stock Photo

RMTXG9R6–Composite of Cassiopeia A supernova remnant across the spectrum: Gamma rays (magenta) Fermi Gamma-ray Space Telescope; X-rays (blue, green) Chandra X-ray Observatory

The Cassiopeia A supernova's first flash of radiation makes six clumps of dust (circled) unusually hot. Cassiopeia A Supernova Flashback Spitzer IR Stock Photo

RMKRJ7GD–The Cassiopeia A supernova's first flash of radiation makes six clumps of dust (circled) unusually hot. Cassiopeia A Supernova Flashback Spitzer IR

Remnants of a Supernova in Cassiopeia Stock Photo

RMD0NY5M–Remnants of a Supernova in Cassiopeia

Supernova Remnant In The Constellation Cassiopeia Showing Shattered Fragments of the dead Star in our Milky Way (Youngest Supernova Remnant in the Milky Way) Stock Photo

RMBKACB6–Supernova Remnant In The Constellation Cassiopeia Showing Shattered Fragments of the dead Star in our Milky Way (Youngest Supernova Remnant in the Milky Way)

Supernova Remnant Cassiopeia A (NASA, Chandra, Hubble, 02/23/11) Stock Photo

RMD3CGAD–Supernova Remnant Cassiopeia A (NASA, Chandra, Hubble, 02/23/11)

A false-colour image of Cassiopeia A, this supernova remnant is located 10,000 light-years away in the constellation Cassiopeia Stock Photo

RM2A6006P–A false-colour image of Cassiopeia A, this supernova remnant is located 10,000 light-years away in the constellation Cassiopeia

Vivid colors and intricate structures of the supernova remnant Cassiopeia A. Stock Photo

RF2RG6DHW–Vivid colors and intricate structures of the supernova remnant Cassiopeia A.

RM2A5YMHD–The many sides of the supernova remnant Cassiopeia A. Located 10,000 light-years away in the northern constellation Cassiopeia, Cassiopeia A is the remnant of a once massive star that died in a violent supernova explosion 325 years ago. Hubble Space Telescope (HST), Spitzer Space Telescope.

The explosion of a star is a dramatic event, but the remains that the star leaves behind can be even more dramatic. A new mid-infrared image from NASA's James Webb Space Telescope provides one stunning example. It shows the supernova remnant Cassiopeia A, created by a stellar explosion 340yrs ago. The image displays vivid colours and intricate structures begging to be examined more closely. Cas A is the youngest known remnant from an exploding, massive star in our galaxy, offering astronomers an opportunity to perform stellar forensics to understand the star's death. Credit: NASA/ESA/CSA Stock Photo

RM2WXE46G–The explosion of a star is a dramatic event, but the remains that the star leaves behind can be even more dramatic. A new mid-infrared image from NASA's James Webb Space Telescope provides one stunning example. It shows the supernova remnant Cassiopeia A, created by a stellar explosion 340yrs ago. The image displays vivid colours and intricate structures begging to be examined more closely. Cas A is the youngest known remnant from an exploding, massive star in our galaxy, offering astronomers an opportunity to perform stellar forensics to understand the star's death. Credit: NASA/ESA/CSA

Cassiopeia A supernova remnants in near infrared light. Stock Photo

RF2TCFH8X–Cassiopeia A supernova remnants in near infrared light.

A detailed view at the tattered remains of a supernova explosion known as Cassiopeia A. Stock Photo

RFD9H47R–A detailed view at the tattered remains of a supernova explosion known as Cassiopeia A.

Supernova Remnant Cassiopeia A from the Hubble Space Telescope Stock Photo

RMA9HGKW–Supernova Remnant Cassiopeia A from the Hubble Space Telescope

Baby Cas A supernova remnant in the constellation Cassiopeia. Stock Photo

RF2X6P2PM–Baby Cas A supernova remnant in the constellation Cassiopeia.

This image, released on December 10, 2023, and taken by NASA's James Webb Space Telescope's NIRCam (Near-Infrared Camera), unveils intricate details of supernova remnant Cassiopeia A (Cas A) and shows the expanding shell of material slamming into the gas shed by the star before it exploded. The most noticeable colors in Webb's newest image are clumps of bright orange and light pink that make up the inner shell of the supernova remnant. These tiny knots of gas, comprised of sulfur, oxygen, argon, and neon from the star itself, are only detectable by NIRCam's exquisite resolution and give resear Stock Photo

RM2TPR5YD–This image, released on December 10, 2023, and taken by NASA's James Webb Space Telescope's NIRCam (Near-Infrared Camera), unveils intricate details of supernova remnant Cassiopeia A (Cas A) and shows the expanding shell of material slamming into the gas shed by the star before it exploded. The most noticeable colors in Webb's newest image are clumps of bright orange and light pink that make up the inner shell of the supernova remnant. These tiny knots of gas, comprised of sulfur, oxygen, argon, and neon from the star itself, are only detectable by NIRCam's exquisite resolution and give resear

Remains of a supernova explosion. Cassiopeia A. Elements of this image furnished by NASA. Stock Photo

RFM53TR0–Remains of a supernova explosion. Cassiopeia A. Elements of this image furnished by NASA.

RM2PMDBR9–The explosion of a star is a dramatic event, but the remains that the star leaves behind can be even more dramatic. A new mid-infrared image from NASA's James Webb Space Telescope provides one stunning example. It shows the supernova remnant Cassiopeia A (Cas A), created by a stellar explosion 340 years ago. The image displays vivid colors and intricate structures begging to be examined more closely. Cas A is the youngest known remnant from an exploding, massive star in our galaxy, offering astronomers an opportunity to perform stellar forensics to understand the star's death.Cassiopeia A (Cas

Cassiopeia A, Supernova Remnant Stock Photo

RMHRJM59–Cassiopeia A, Supernova Remnant

RMD991T6–Composite of Cassiopeia A supernova remnant across the spectrum: Gamma rays (magenta) Fermi Gamma-ray Space Telescope; X-rays (blue, green) Chandra X-ray Observatory; visible light (yellow) from the Hubble Telescope. Science

This June 9, 2005 NASA false-color picture shows the supernova remnant of Cassiopeia A. This image is made up of images taken by NASA's, Spitzer Space Telescope, Hubble Space Telescope and the Chandra X-ray Observatory. UPI/NASA Stock Photo

RMW0MG08–This June 9, 2005 NASA false-color picture shows the supernova remnant of Cassiopeia A. This image is made up of images taken by NASA's, Spitzer Space Telescope, Hubble Space Telescope and the Chandra X-ray Observatory. UPI/NASA

RMG1CBRM–A false-colour image of Cassiopeia A, this supernova remnant is located 10,000 light-years away in the constellation Cassiopeia

This image from NASA's Spitzer Space Telescope highlights dramatic changes in phenomena referred to as light echoes (colored areas) around the Cassiopeia A supernova remnant (center). Cassiopeia A is the remnant of a once massive star that died in a violent supernova explosion. It consists of a dead star, called a neutron star, and a surrounding shell of material that was blasted off as the star died. A light echo is created when a star explodes or erupts, flashing light into surrounding clumps of dust. As the light zips through the dust clumps, it heats them up, causing them to glow successi Stock Photo

RMKRJ7G5–This image from NASA's Spitzer Space Telescope highlights dramatic changes in phenomena referred to as light echoes (colored areas) around the Cassiopeia A supernova remnant (center). Cassiopeia A is the remnant of a once massive star that died in a violent supernova explosion. It consists of a dead star, called a neutron star, and a surrounding shell of material that was blasted off as the star died. A light echo is created when a star explodes or erupts, flashing light into surrounding clumps of dust. As the light zips through the dust clumps, it heats them up, causing them to glow successi

False-colour image of supernova remnant Cassiopeia A in constellation Cassiopeia, 10,000 light-years away. It is the remnant of a once massive star that died in a supernova explosion. Credit NASA. Science Astronomy Stock Photo

RMD991PF–False-colour image of supernova remnant Cassiopeia A in constellation Cassiopeia, 10,000 light-years away. It is the remnant of a once massive star that died in a supernova explosion. Credit NASA. Science Astronomy

RMD0NY4H–Aftermath of a Supernova

Supernova Remnant Cassiopeia A (NASA, Chandra, 1/6/09) Stock Photo

RMD3AMBP–Supernova Remnant Cassiopeia A (NASA, Chandra, 1/6/09)

This beautiful bulb might look like a Christmas ornament but it is the blown-out remains of a stellar explosion, or supernova. The remains, called Cassiopeia A, are shown here in an infrared composite from NASA's Spitzer Space Telescope. Silicon gas is blue and argon gas is green, while red represents about 10,000 Earth masses worth of dust. Yellow shows areas where red and green overlap. The fact that the red and green do overlap indicates that this supernova is synthesizing dust and gas together. This is the smoking gun indicating that supernovae were significant suppliers of fresh dust in Stock Photo

RMKRF88D–This beautiful bulb might look like a Christmas ornament but it is the blown-out remains of a stellar explosion, or supernova. The remains, called Cassiopeia A, are shown here in an infrared composite from NASA's Spitzer Space Telescope. Silicon gas is blue and argon gas is green, while red represents about 10,000 Earth masses worth of dust. Yellow shows areas where red and green overlap. The fact that the red and green do overlap indicates that this supernova is synthesizing dust and gas together. This is the smoking gun indicating that supernovae were significant suppliers of fresh dust in

A new image taken with NASA's Hubble Space Telescope provides a detailed look at the tattered remains of a supernova explosion known as Cassiopeia A (Cas A) on August 29, 2006. It is the youngest known remnant from a supernova explosion in the Milky Way. The new Hubble image shows the complex and intricate structure of the star's shattered fragments. The image is a composite made from 18 separate images taken in December 2004 using Hubble's Advanced Camera for Surveys (ACS). (UPI Photo/NASA/ESA/HUBBLE HERITAGE) Stock Photo

RMW0M9K3–A new image taken with NASA's Hubble Space Telescope provides a detailed look at the tattered remains of a supernova explosion known as Cassiopeia A (Cas A) on August 29, 2006. It is the youngest known remnant from a supernova explosion in the Milky Way. The new Hubble image shows the complex and intricate structure of the star's shattered fragments. The image is a composite made from 18 separate images taken in December 2004 using Hubble's Advanced Camera for Surveys (ACS). (UPI Photo/NASA/ESA/HUBBLE HERITAGE)

The Cassiopeia A supernova's first flash of radiation makes six clumps of dust (circled in annotated version) unusually hot. The supernova remnant is the large white ball in the center. This infrared picture was taken by NASA's Spitzer Space Telescope. Stock Photo

RM2A5YMM6–The Cassiopeia A supernova's first flash of radiation makes six clumps of dust (circled in annotated version) unusually hot. The supernova remnant is the large white ball in the center. This infrared picture was taken by NASA's Spitzer Space Telescope.

This Spitzer Space Telescope composite shows the supernova remnant Cassiopeia A (white ball) and surrounding clouds of dust (gray, orange and blue). It consists of two processed images taken one year apart. Dust features that have not changed over time appear gray, while those that have changed are colored blue or orange. Blue represents an earlier time and orange, a later time. These observations illustrate that a blast of light from Cassiopeia A is waltzing outward through the dusty skies. This dance, called an 'infrared echo,' began when the remnant erupted about 50 years ago. Cassiopeia Stock Photo

RMKRJ7EE–This Spitzer Space Telescope composite shows the supernova remnant Cassiopeia A (white ball) and surrounding clouds of dust (gray, orange and blue). It consists of two processed images taken one year apart. Dust features that have not changed over time appear gray, while those that have changed are colored blue or orange. Blue represents an earlier time and orange, a later time. These observations illustrate that a blast of light from Cassiopeia A is waltzing outward through the dusty skies. This dance, called an 'infrared echo,' began when the remnant erupted about 50 years ago. Cassiopeia

The tattered remains of a supernova explosion known as Cassiopeia A. It is the youngest known remnant from a supernova explosion in the Milky Way. Ele Stock Photo

RFJXMB62–The tattered remains of a supernova explosion known as Cassiopeia A. It is the youngest known remnant from a supernova explosion in the Milky Way. Ele

Space. 14th Jan, 2024. For the first time, astronomers have combined data from NASA's Chandra X-ray Observatory and James Webb Space Telescope to study the well-known supernova remnant Cassiopeia A (Cas A). This work has helped explain an unusual structure in the debris from the destroyed star called the 'Green Monster' because of its resemblance to the wall in the left field of Fenway Park. (Credit Image: © NASA/ESA/STScl/ZUMA Press Wire) EDITORIAL USAGE ONLY! Not for Commercial USAGE! Stock Photo

RM2WD49NW–Space. 14th Jan, 2024. For the first time, astronomers have combined data from NASA's Chandra X-ray Observatory and James Webb Space Telescope to study the well-known supernova remnant Cassiopeia A (Cas A). This work has helped explain an unusual structure in the debris from the destroyed star called the 'Green Monster' because of its resemblance to the wall in the left field of Fenway Park. (Credit Image: © NASA/ESA/STScl/ZUMA Press Wire) EDITORIAL USAGE ONLY! Not for Commercial USAGE!

Remains of a supernova explosion. Cassiopeia A. Elements of this image furnished by NASA. Retouched image. Stock Photo

RFM53W0D–Remains of a supernova explosion. Cassiopeia A. Elements of this image furnished by NASA. Retouched image.

Space. 21st Oct, 2022. When a massive star collapsed in the Cassiopeia constellation, it generated a supernova explosion with some of the fastest shockwaves in the Milky Way. These speedy shock waves are one of the reasons the Cassiopeia A (Cas A) supernova remnant was chosen to be our Imaging X-ray Polarimetry Explorer's (IXPE) first observed object. This composite image, made of data from IXPE, the Chandra Observatory, and the Hubble Telescope, shows Cas A. IXPE's investigation of Cas A from Jan. 11 to Jan. 29, 2022, added crucial information about the behavior of exploded stars magnetic f Stock Photo

RM2K89GNE–Space. 21st Oct, 2022. When a massive star collapsed in the Cassiopeia constellation, it generated a supernova explosion with some of the fastest shockwaves in the Milky Way. These speedy shock waves are one of the reasons the Cassiopeia A (Cas A) supernova remnant was chosen to be our Imaging X-ray Polarimetry Explorer's (IXPE) first observed object. This composite image, made of data from IXPE, the Chandra Observatory, and the Hubble Telescope, shows Cas A. IXPE's investigation of Cas A from Jan. 11 to Jan. 29, 2022, added crucial information about the behavior of exploded stars magnetic f

RMB1G8YP–Explosion in Space

Space. 7th Apr, 2023. The explosion of a star is a dramatic event, but the remains the star leaves behind can be even more dramatic. A new mid-infrared image from NASA's James Webb Space Telescope provides one stunning example. It shows the supernova remnant Cassiopeia A (Cas A), created by a stellar explosion 340 years ago from Earth's perspective. Cas A is the youngest known remnant from an exploding, massive star in our galaxy. Cassiopeia A (Cas A) is a supernova remnant located about 11,000 light-years from Earth in the constellation Cassiopeia. It spans approximately 10 light-years. Thi Stock Photo

RM2PKGKYR–Space. 7th Apr, 2023. The explosion of a star is a dramatic event, but the remains the star leaves behind can be even more dramatic. A new mid-infrared image from NASA's James Webb Space Telescope provides one stunning example. It shows the supernova remnant Cassiopeia A (Cas A), created by a stellar explosion 340 years ago from Earth's perspective. Cas A is the youngest known remnant from an exploding, massive star in our galaxy. Cassiopeia A (Cas A) is a supernova remnant located about 11,000 light-years from Earth in the constellation Cassiopeia. It spans approximately 10 light-years. Thi

Cassiopeia A, Supernova Remnant, Composite Stock Photo

RMHRJEG9–Cassiopeia A, Supernova Remnant, Composite

RMD99A4X–The many sides of the supernova remnant Cassiopeia A. Located 10,000 light-years away in the northern constellation Cassiopeia, Cassiopeia A is the remnant of a once massive star that died in a violent supernova explosion 325 years ago. Hubble Space Telescope (HST), Spitzer Space Telescope.

A Star Explodes, Turns Inside-Out (NASA, Chandra, Spitzer, 03/29/12) Stock Photo

RMD3DBF6–A Star Explodes, Turns Inside-Out (NASA, Chandra, Spitzer, 03/29/12)

Cassiopeia A Chandra Discovers Relativistic Pinball Machine 2940633609 o Stock Photo

RMKYMPRG–Cassiopeia A Chandra Discovers Relativistic Pinball Machine 2940633609 o

RMTXG95G–False-colour image of supernova remnant Cassiopeia A in constellation Cassiopeia, 10,000 light-years away. It is the remnant of a once massive star that died in a supernova explosion Credit NASA

These beautiful bulbs might look like they belong on Christmas trees, but they are actually different Spitzer Space Telescope views of the blown-out remains of a stellar explosion, or supernova. Called Cassiopeia A, this supernova remnant is located about 10,000 light-years away in our own Milky Way galaxy. The upper left panel is a composite made up of three infrared views shown in the remaining panels. The bottom left view shows argon gas (green) that was synthesized as it was ejected from the star. The bottom right view shows a collection of dust (red), including proto-silicates, silicate Stock Photo

RMKRJ7FW–These beautiful bulbs might look like they belong on Christmas trees, but they are actually different Spitzer Space Telescope views of the blown-out remains of a stellar explosion, or supernova. Called Cassiopeia A, this supernova remnant is located about 10,000 light-years away in our own Milky Way galaxy. The upper left panel is a composite made up of three infrared views shown in the remaining panels. The bottom left view shows argon gas (green) that was synthesized as it was ejected from the star. The bottom right view shows a collection of dust (red), including proto-silicates, silicate

Cassiopeia A Cassiopeia A in Many Colors 2941486784 o Stock Photo

RMKYMJYR–Cassiopeia A Cassiopeia A in Many Colors 2941486784 o

RFJP1RA1–The tattered remains of a supernova explosion known as Cassiopeia A. It is the youngest known remnant from a supernova explosion in the Milky Way. Ele

Cassiopeia A: Chandra Discovers Relativistic Pinball Machine Stock Photo

RMD5DYCD–Cassiopeia A: Chandra Discovers Relativistic Pinball Machine

RFK4Y8TP–The tattered remains of a supernova explosion known as Cassiopeia A. It is the youngest known remnant from a supernova explosion in the Milky Way. Ele

Supernova Core pulsar neutron star. Remains of a supernova explosion. Elements of this image furnished by NASA. Retouched image. Stock Photo

RF2E6GECY–Supernova Core pulsar neutron star. Remains of a supernova explosion. Elements of this image furnished by NASA. Retouched image.

Cassiopeia A, Supernova Remnant, Optical Stock Photo

RMHRJCDP–Cassiopeia A, Supernova Remnant, Optical

RMD99A55–The many sides of the supernova remnant Cassiopeia A. Located 10,000 light-years away in the northern constellation Cassiopeia, Cassiopeia A is the remnant of a once massive star that died in a violent supernova explosion 325 years ago. Hubble Space Telescope (HST), Spitzer Space Telescope.

RMKRE9EA–Supernova cassiopeia-a

RMD3RFH3–Cassiopeia A: Chandra Discovers Relativistic Pinball Machine

RFJM1704–The tattered remains of a supernova explosion known as Cassiopeia A. It is the youngest known remnant from a supernova explosion in the Milky Way. Ele

Cassiopeia A: Cassiopeia A in Many Colors Stock Photo

RMD5DYEE–Cassiopeia A: Cassiopeia A in Many Colors

RMHRJCDR–Cassiopeia A, Supernova Remnant, Composite

RMD99ABR–The Cassiopeia A supernova's first flash of radiation makes six clumps of dust (circled in annotated version) unusually hot. The supernova remnant is the large white ball in the center. This infrared picture was taken by NASA's Spitzer Space Telescope.

HEAO-2 Image of the Supernova Remnant Cassiopeia A Taken by the High Energy Astronomy Observatory 8003547 Stock Photo

RMKRNARN–HEAO-2 Image of the Supernova Remnant Cassiopeia A Taken by the High Energy Astronomy Observatory 8003547

RMD3RFW8–Cassiopeia A: Cassiopeia A in Many Colors

Carbon Atmosphere Discovered on Neutron Star (NASA, Chandra, 11/04/09) Stock Photo

RMD3CCAY–Carbon Atmosphere Discovered on Neutron Star (NASA, Chandra, 11/04/09)

RMHRJN2H–Cassiopeia A, Supernova Remnant

RMD99ABT–The Cassiopeia A supernova's first flash of radiation makes six clumps of dust (circled in annotated version) unusually hot. The supernova remnant is the large white ball in the center. This infrared picture was taken by NASA's Spitzer Space Telescope.

IDL TIFF file Cas A Supernova Remnant J. Morse (U.CO) HST WFPC2 B (F450W), R (F675W), IR (F850LP) Details of Supernova Remnant Cassiopeia A - Hubble Stock Photo

RMKRE1WY–IDL TIFF file Cas A Supernova Remnant J. Morse (U.CO) HST WFPC2 B (F450W), R (F675W), IR (F850LP) Details of Supernova Remnant Cassiopeia A - Hubble

Superfluid in Neutron Star's Core (NASA, Chandra, Hubble, 02/23/11) Stock Photo

RMD3CGA7–Superfluid in Neutron Star's Core (NASA, Chandra, Hubble, 02/23/11)

Cassiopeia A, Supernova Remnant, X-Ray Stock Photo

RMHRJMAK–Cassiopeia A, Supernova Remnant, X-Ray

For the first time, a multiwavelength three-dimensional reconstruction of a supernova remnant has been created. This stunning Stock Photo

RMD98BE6–For the first time, a multiwavelength three-dimensional reconstruction of a supernova remnant has been created. This stunning

This X-ray image of the Cassiopeia A (Cas A) supernova remnant is the official first light image of the Chandra X-ray Observatory. The 5,000 second image was made with the Advanced CCD Imaging Spectrometer (ACIS). Two shock waves are visible: a fast outer shock and a slower inner shock. The inner shock wave is believed to be due to the collision of the ejecta from the supernova explosion with a circumstellar shell of material, heating it to a temperature of ten million degrees Celsius. The outer shock wave is analogous to an awesome sonic boom resulting from this collision. The bright object n Stock Photo

RMKRFB0F–This X-ray image of the Cassiopeia A (Cas A) supernova remnant is the official first light image of the Chandra X-ray Observatory. The 5,000 second image was made with the Advanced CCD Imaging Spectrometer (ACIS). Two shock waves are visible: a fast outer shock and a slower inner shock. The inner shock wave is believed to be due to the collision of the ejecta from the supernova explosion with a circumstellar shell of material, heating it to a temperature of ten million degrees Celsius. The outer shock wave is analogous to an awesome sonic boom resulting from this collision. The bright object n