18 images found for "chandra x-ray telescope"
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The images at the top of this graphic represent two popular models describing how stars blast apart. The models point to different triggers of the explosion. Jet-driven models are illustrated with an artist's concept shown at left.
The images at the top of this graphic represent two popular models describing how stars blast apart. The models point to different triggers of the explosion. Jet-driven models are illustrated with an artist's concept shown at left.

NuSTAR Data Point to Sloshing Supernovas

The images at the top of this graphic represent two popular models describing how stars blast apart. The models point to different triggers of the explosion. Jet-driven models are illustrated with an artist's concept shown at left.

Mission: Chandra X-ray Observatory, NuSTAR
Instrument: Chandra X-ray Telescope, Nuclear Spectroscopic Telescope Array
Size: 3000 x 2400
ID#: PIA17846
Added: 2014-02-19

Views: 447

NuSTAR Data Point to Sloshing Supernovas

The images at the top of this graphic represent two popular models describing how stars blast apart. The models point to different triggers of the explosion. Jet-driven models are illustrated with an artist's concept shown at left.

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A massive star (left), which has created elements as heavy as iron in its interior, blows up in a tremendous explosion (middle), scattering its outer layers in a structure called a supernova remnant (right).
A massive star (left), which has created elements as heavy as iron in its interior, blows up in a tremendous explosion (middle), scattering its outer layers in a structure called a supernova remnant (right).

Evolution of a Supernova

A massive star (left), which has created elements as heavy as iron in its interior, blows up in a tremendous explosion (middle), scattering its outer layers in a structure called a supernova remnant (right).

Mission: Chandra X-ray Observatory, NuSTAR
Instrument: Chandra X-ray Telescope, Nuclear Spectroscopic Telescope Array
Size: 3000 x 2000
ID#: PIA17844
Added: 2014-02-19

Views: 530

Evolution of a Supernova

A massive star (left), which has created elements as heavy as iron in its interior, blows up in a tremendous explosion (middle), scattering its outer layers in a structure called a supernova remnant (right).

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When astronomers first looked at images of a supernova remnant called Cassiopeia A, captured by NASA's NuSTAR. The mystery of Cassiopeia A (Cas A), a massive star that exploded in a supernova more than 11,000 years ago continues to confound scientists.
When astronomers first looked at images of a supernova remnant called Cassiopeia A, captured by NASA's NuSTAR. The mystery of Cassiopeia A (Cas A), a massive star that exploded in a supernova more than 11,000 years ago continues to confound scientists.

The Case of Missing Iron in Cassiopeia A

When astronomers first looked at images of a supernova remnant called Cassiopeia A, captured by NASA's NuSTAR. The mystery of Cassiopeia A (Cas A), a massive star that exploded in a supernova more than 11,000 years ago continues to confound scientists.

Mission: Chandra X-ray Observatory, NuSTAR
Instrument: Chandra X-ray Telescope, Nuclear Spectroscopic Telescope Array
Size: 2048 x 1024
ID#: PIA17842
Added: 2014-02-19

Views: 380

The Case of Missing Iron in Cassiopeia A

When astronomers first looked at images of a supernova remnant called Cassiopeia A, captured by NASA's NuSTAR. The mystery of Cassiopeia A (Cas A), a massive star that exploded in a supernova more than 11,000 years ago continues to confound scientists.

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NASA's NuSTAR has, for the first time, imaged the radioactive 'guts' of a supernova remnant, the leftover remains of a star that exploded. The NuSTAR data are blue, and show high-energy X-rays.
NASA's NuSTAR has, for the first time, imaged the radioactive 'guts' of a supernova remnant, the leftover remains of a star that exploded. The NuSTAR data are blue, and show high-energy X-rays.

Radioactive Core of a Dead Star

NASA's NuSTAR has, for the first time, imaged the radioactive 'guts' of a supernova remnant, the leftover remains of a star that exploded. The NuSTAR data are blue, and show high-energy X-rays.

Mission: Chandra X-ray Observatory, NuSTAR
Instrument: Chandra X-ray Telescope, Nuclear Spectroscopic Telescope Array
Size: 1024 x 1024
ID#: PIA17841
Added: 2014-02-19

Views: 1024

Radioactive Core of a Dead Star

NASA's NuSTAR has, for the first time, imaged the radioactive 'guts' of a supernova remnant, the leftover remains of a star that exploded. The NuSTAR data are blue, and show high-energy X-rays.

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NASA's NuSTAR is complementing previous observations of the Cassiopeia A supernova remnant (red and green) by providing the first maps of radioactive material forged in the fiery explosion (blue).
NASA's NuSTAR is complementing previous observations of the Cassiopeia A supernova remnant (red and green) by providing the first maps of radioactive material forged in the fiery explosion (blue).

Adding a New 'Color' to Palate of Cassiopeia A Images

NASA's NuSTAR is complementing previous observations of the Cassiopeia A supernova remnant (red and green) by providing the first maps of radioactive material forged in the fiery explosion (blue).

Mission: Chandra X-ray Observatory, NuSTAR
Instrument: Chandra X-ray Telescope, Nuclear Spectroscopic Telescope Array
Size: 3072 x 1024
ID#: PIA17839
Added: 2014-02-19

Views: 707

Adding a New 'Color' to Palate of Cassiopeia A Images

NASA's NuSTAR is complementing previous observations of the Cassiopeia A supernova remnant (red and green) by providing the first maps of radioactive material forged in the fiery explosion (blue).

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This is the first map of radioactivity in a supernova remnant, the blown-out bits and pieces of a massive star that exploded. The blue color shows radioactive material mapped in high-energy X-rays using NASA's NuSTAR.
This is the first map of radioactivity in a supernova remnant, the blown-out bits and pieces of a massive star that exploded. The blue color shows radioactive material mapped in high-energy X-rays using NASA's NuSTAR.

Untangling the Remains of Cassiopeia A

This is the first map of radioactivity in a supernova remnant, the blown-out bits and pieces of a massive star that exploded. The blue color shows radioactive material mapped in high-energy X-rays using NASA's NuSTAR.

Mission: Chandra X-ray Observatory, NuSTAR
Instrument: Chandra X-ray Telescope, Nuclear Spectroscopic Telescope Array
Size: 3000 x 3000
ID#: PIA17838
Added: 2014-02-19

Views: 5156

Untangling the Remains of Cassiopeia A

This is the first map of radioactivity in a supernova remnant, the blown-out bits and pieces of a massive star that exploded. The blue color shows radioactive material mapped in high-energy X-rays using NASA's NuSTAR.

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The tip of the 'wing' of the Small Magellanic Cloud galaxy is dazzling in this new view from NASA's Great Observatories. The SMC, is a small galaxy about 200,000 light-years way that orbits our own Milky Way spiral galaxy.
The tip of the 'wing' of the Small Magellanic Cloud galaxy is dazzling in this new view from NASA's Great Observatories. The SMC, is a small galaxy about 200,000 light-years way that orbits our own Milky Way spiral galaxy.

Taken Under the 'Wing' of the Small Magellanic Cloud

The tip of the 'wing' of the Small Magellanic Cloud galaxy is dazzling in this new view from NASA's Great Observatories. The SMC, is a small galaxy about 200,000 light-years way that orbits our own Milky Way spiral galaxy.

Mission: Chandra X-ray Observatory, Hubble Space Telescope, Spitzer Space Telescope
Instrument: Chandra X-ray Telescope, Infrared Array Camera (IRAC), Visible-Light
Size: 3600 x 3600
ID#: PIA16884
Added: 2013-04-03

Views: 35228

Taken Under the 'Wing' of the Small Magellanic Cloud

The tip of the 'wing' of the Small Magellanic Cloud galaxy is dazzling in this new view from NASA's Great Observatories. The SMC, is a small galaxy about 200,000 light-years way that orbits our own Milky Way spiral galaxy.

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About 2,400 massive stars in the center of 30 Doradus, the Tarantula Nebula, produce intense radiation and powerful winds as they blow off material seen as infrared emission from NASA's Spitzer Space Telescope and X-rays from Chandra X-ray Observatory.
About 2,400 massive stars in the center of 30 Doradus, the Tarantula Nebula, produce intense radiation and powerful winds as they blow off material seen as infrared emission from NASA's Spitzer Space Telescope and X-rays from Chandra X-ray Observatory.

30 Doradus: The Growing Tarantula Within

About 2,400 massive stars in the center of 30 Doradus, the Tarantula Nebula, produce intense radiation and powerful winds as they blow off material seen as infrared emission from NASA's Spitzer Space Telescope and X-rays from Chandra X-ray Observatory.

Mission: Chandra X-ray Observatory, Spitzer Space Telescope
Instrument: Chandra X-ray Telescope, Infrared Array Camera (IRAC)
Size: 3600 x 3069
ID#: PIA15079
Added: 2011-11-16

Views: 9472

30 Doradus: The Growing Tarantula Within

About 2,400 massive stars in the center of 30 Doradus, the Tarantula Nebula, produce intense radiation and powerful winds as they blow off material seen as infrared emission from NASA's Spitzer Space Telescope and X-rays from Chandra X-ray Observatory.

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This composite image of the star cluster NGC 28 contains X-ray data from Chandra, in purple, with infrared observations from Spitzer, in red, green, blue. NGC 281 is known informally as the 'Pacman Nebula' because of its appearance in optical images.
This composite image of the star cluster NGC 28 contains X-ray data from Chandra, in purple, with infrared observations from Spitzer, in red, green, blue. NGC 281 is known informally as the 'Pacman Nebula' because of its appearance in optical images.

The 'Pacman Nebula'

This composite image of the star cluster NGC 28 contains X-ray data from Chandra, in purple, with infrared observations from Spitzer, in red, green, blue. NGC 281 is known informally as the 'Pacman Nebula' because of its appearance in optical images.

Target: NGC 281
Mission: Chandra X-Ray Telescope, Spitzer Space Telescope
Spacecraft: Chandra X-Ray Telescope, Spitzer Space Telescope
Instrument: Chandra X-Ray Telescope, Infrared Array Camera (IRAC)
Size: 3600 x 2719
ID#: PIA14731
Added: 2011-09-28

Views: 7542

The 'Pacman Nebula'

This composite image of the star cluster NGC 28 contains X-ray data from Chandra, in purple, with infrared observations from Spitzer, in red, green, blue. NGC 281 is known informally as the 'Pacman Nebula' because of its appearance in optical images.

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A composite image from NASA's Chandra and Spitzer space telescopes shows the dusty remains of a collapsed star, a supernova remnant called G54.1+0.3. The white source at the center is a dead star called a pulsar.
A composite image from NASA's Chandra and Spitzer space telescopes shows the dusty remains of a collapsed star, a supernova remnant called G54.1+0.3. The white source at the center is a dead star called a pulsar.

Dusty Dead Star

A composite image from NASA's Chandra and Spitzer space telescopes shows the dusty remains of a collapsed star, a supernova remnant called G54.1+0.3. The white source at the center is a dead star called a pulsar.

Mission: Chandra X-ray Observatory, Spitzer Space Telescope
Spacecraft: Chandra X-ray Telescope, Spitzer Space Telescope
Instrument: Chandra X-ray Telescope, Infrared Array Camera (IRAC)
Size: 3600 x 3547
ID#: PIA12982
Added: 2010-03-29

Views: 4502

Dusty Dead Star

A composite image from NASA's Chandra and Spitzer space telescopes shows the dusty remains of a collapsed star, a supernova remnant called G54.1+0.3. The white source at the center is a dead star called a pulsar.

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This composite image, combining data from NASA's Chandra X-ray Observatory and Spitzer Space Telescope shows the star-forming cloud Cepheus B, located in our Milky Way galaxy about 2,400 light years from Earth
This composite image, combining data from NASA's Chandra X-ray Observatory and Spitzer Space Telescope shows the star-forming cloud Cepheus B, located in our Milky Way galaxy about 2,400 light years from Earth

Trigger-Happy Cloud

This composite image, combining data from NASA's Chandra X-ray Observatory and Spitzer Space Telescope shows the star-forming cloud Cepheus B, located in our Milky Way galaxy about 2,400 light years from Earth

Target: Cepheus B
Mission: Chandra X-ray Observatory, Spitzer Space Telescope
Spacecraft: Chandra X-ray Telescope, Spitzer Space Telescope
Instrument: Chandra X-ray Telescope, Infrared Array Camera (IRAC)
Size: 2749 x 3600
ID#: PIA12169
Added: 2009-08-12

Views: 5669

Trigger-Happy Cloud

This composite image, combining data from NASA's Chandra X-ray Observatory and Spitzer Space Telescope shows the star-forming cloud Cepheus B, located in our Milky Way galaxy about 2,400 light years from Earth

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NASA's Great Observatories continue Galileo's legacy with stunning images and breakthrough science from the Hubble Space Telescope, the Spitzer Space Telescope, and the Chandra X-ray Observatory.
NASA's Great Observatories continue Galileo's legacy with stunning images and breakthrough science from the Hubble Space Telescope, the Spitzer Space Telescope, and the Chandra X-ray Observatory.

NASA's Great Observatories Celebrate the International Year of Astronomy

NASA's Great Observatories continue Galileo's legacy with stunning images and breakthrough science from the Hubble Space Telescope, the Spitzer Space Telescope, and the Chandra X-ray Observatory.

Target: Messier 101
Mission: Hubble Space Telescope, Spitzer Space Telescope
Spacecraft: Hubble Space Telescope, Spitzer Space Telescope
Instrument: Chandra X-ray Telescope, Infrared Array Camera (IRAC), Visible Light
Size: 7200 x 7200
ID#: PIA11797
Added: 2009-02-10

Views: 5888

NASA's Great Observatories Celebrate the International Year of Astronomy

NASA's Great Observatories continue Galileo's legacy with stunning images and breakthrough science from the Hubble Space Telescope, the Spitzer Space Telescope, and the Chandra X-ray Observatory.

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For the first time, a multiwavelength three-dimensional reconstruction of a supernova remnant has been created. This visualization of Cassiopeia A, or Cas A, the result of an explosion approximately 330 years ago, uses data from several NASA telescopes.
For the first time, a multiwavelength three-dimensional reconstruction of a supernova remnant has been created. This visualization of Cassiopeia A, or Cas A, the result of an explosion approximately 330 years ago, uses data from several NASA telescopes.

Supernova Remnant in 3-D

For the first time, a multiwavelength three-dimensional reconstruction of a supernova remnant has been created. This visualization of Cassiopeia A, or Cas A, the result of an explosion approximately 330 years ago, uses data from several NASA telescopes.

Target: Cassiopeia A
Mission: Chandra X-ray Observatory, Spitzer Space Telescope
Spacecraft: Chandra X-ray Telescope, Spitzer Space Telescope
Instrument: Chandra X-ray Telescope, Infrared Array Camera (IRAC)
Size: 719 x 479
ID#: PIA11748
Added: 2009-01-06

Views: 5508

Supernova Remnant in 3-D

For the first time, a multiwavelength three-dimensional reconstruction of a supernova remnant has been created. This visualization of Cassiopeia A, or Cas A, the result of an explosion approximately 330 years ago, uses data from several NASA telescopes.

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This composite image shows the Coronet in X-rays from Chandra and infrared from NASA's Spitzer Space Telescope (orange, green, and cyan). The Spitzer data show young stars plus diffuse emission from dust.
This composite image shows the Coronet in X-rays from Chandra and infrared from NASA's Spitzer Space Telescope (orange, green, and cyan). The Spitzer data show young stars plus diffuse emission from dust.

Coronet: A Star-Formation Neighbor

This composite image shows the Coronet in X-rays from Chandra and infrared from NASA's Spitzer Space Telescope (orange, green, and cyan). The Spitzer data show young stars plus diffuse emission from dust.

Mission: Spitzer Space Telescope
Spacecraft: Spitzer Space Telescope
Instrument: Infrared Array Camera (IRAC), Chandra X-Ray Telescope
Size: 3300 x 3300
ID#: PIA09925
Added: 2007-09-13

Views: 5525

Coronet: A Star-Formation Neighbor

This composite image shows the Coronet in X-rays from Chandra and infrared from NASA's Spitzer Space Telescope (orange, green, and cyan). The Spitzer data show young stars plus diffuse emission from dust.

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NASA's Spitzer, Hubble and Chandra space observatories teamed up to create this multi-wavelength, false-colored view of the M82 galaxy. The lively 
portrait celebrates Hubble's 'sweet sixteen' birthday.
NASA's Spitzer, Hubble and Chandra space observatories teamed up to create this multi-wavelength, false-colored view of the M82 galaxy. The lively 
portrait celebrates Hubble's 'sweet sixteen' birthday.

Great Observatories Present Rainbow of a Galaxy

NASA's Spitzer, Hubble and Chandra space observatories teamed up to create this multi-wavelength, false-colored view of the M82 galaxy. The lively 
portrait celebrates Hubble's 'sweet sixteen' birthday.

Target: M82 Galaxy
Mission: Hubble Space Telescope (HST), Spitzer Space Telescope
Spacecraft: Spitzer Space Telescope
Instrument: Chandra X-ray Telescope, Infrared Array Camera (IRAC), Visible Light
Size: 4299 x 3490
ID#: PIA08093
Added: 2006-04-24

Views: 7603

Great Observatories Present Rainbow of a Galaxy

NASA's Spitzer, Hubble and Chandra space observatories teamed up to create this multi-wavelength, false-colored view of the M82 galaxy. The lively portrait celebrates Hubble's 'sweet sixteen' birthday.

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This false-color composite image shows the Cartwheel galaxy, where the first ripple appears as an ultraviolet-bright blue outer ring.
This false-color composite image shows the Cartwheel galaxy, where the first ripple appears as an ultraviolet-bright blue outer ring.

A Stellar Ripple

This false-color composite image shows the Cartwheel galaxy, where the first ripple appears as an ultraviolet-bright blue outer ring.

Target: Cartwheel Galaxy
Mission: Galaxy Evolution Explorer (GALEX), Hubble Space Telescope (HST), Spitzer Space Telescope
Spacecraft: GALEX Orbiter, Hubble Space Telescope (HST), Spitzer Space Telescope
Instrument: Chandra X-ray Telescope, GALEX Telescope, Infrared Array Camera (IRAC), Visible Light
Size: 1500 x 1500
ID#: PIA03296
Added: 2006-01-11

Views: 7811

A Stellar Ripple

This false-color composite image shows the Cartwheel galaxy, where the first ripple appears as an ultraviolet-bright blue outer ring.

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This false-color image from three of NASA's Great Observatories provides one example of a star that died in a fiery supernova blast. Called Cassiopeia A, this supernova remnant is located 10,000 light-years away in the constellation Cassiopeia.
This false-color image from three of NASA's Great Observatories provides one example of a star that died in a fiery supernova blast. Called Cassiopeia A, this supernova remnant is located 10,000 light-years away in the constellation Cassiopeia.

Cassiopeia A: Death Becomes Her

This false-color image from three of NASA's Great Observatories provides one example of a star that died in a fiery supernova blast. Called Cassiopeia A, this supernova remnant is located 10,000 light-years away in the constellation Cassiopeia.

Target: Cassiopeia A
Mission: Hubble Space Telescope (HST), Spitzer Space Telescope
Spacecraft: Hubble Space Telescope, Spitzer Space Telescope
Instrument: Infrared Array Camera (IRAC), Visible Light, Chandra X-ray Telescope
Size: 1835 x 1348
ID#: PIA03519
Added: 2005-06-10

Views: 37262

Cassiopeia A: Death Becomes Her

This false-color image from three of NASA's Great Observatories provides one example of a star that died in a fiery supernova blast. Called Cassiopeia A, this supernova remnant is located 10,000 light-years away in the constellation Cassiopeia.

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NASA's three Great Observatories -- the Hubble Space Telescope, the SpitzerSpace Telescope, and the Chandra X-ray Observatory -- joined forces to probe theexpanding remains of a supernova, called Kepler's supernova remnant.
NASA's three Great Observatories -- the Hubble Space Telescope, the SpitzerSpace Telescope, and the Chandra X-ray Observatory -- joined forces to probe theexpanding remains of a supernova, called Kepler's supernova remnant.

Three Great Eyes on Kepler's Supernova Remnant

NASA's three Great Observatories -- the Hubble Space Telescope, the SpitzerSpace Telescope, and the Chandra X-ray Observatory -- joined forces to probe theexpanding remains of a supernova, called Kepler's supernova remnant.

Mission: Hubble Space Telescope (HST), Spitzer Space Telescope
Spacecraft: Hubble Space Telescope, Spitzer Space Telescope
Instrument: Chandra X-Ray Telescope, Hubble Space Telescope, Spitzer Space Telescope
Size: 750 x 750
ID#: PIA06907
Added: 2004-10-06

Views: 6494

Three Great Eyes on Kepler's Supernova Remnant

NASA's three Great Observatories -- the Hubble Space Telescope, the SpitzerSpace Telescope, and the Chandra X-ray Observatory -- joined forces to probe theexpanding remains of a supernova, called Kepler's supernova remnant.

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