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Recent discoveries and updates of the Chandra mission in video and audio formats.
G327.1-1.1 in 60 Seconds
G327.1-1.1 is the aftermath of a massive star that exploded as a supernova in the Milky Way galaxy.
- Related Links:
-- Pushing the Envelope
-- Tour of G327.1-1.1
G327.1-1.1 is the aftermath of a massive star that exploded as a supernova in the Milky Way galaxy.
- Related Links:
-- Pushing the Envelope
-- Tour of G327.1-1.1
G54.1+0.3 in 60 Seconds
Data from the Chandra X-ray Observatory and the Spitzer Space Telescope were combined to create this image of the dusty remains of a collapsed star.
- Related Links:
-- Ashes to Ashes, Dust to Dust
-- Tour of G54.1+0.3
Data from the Chandra X-ray Observatory and the Spitzer Space Telescope were combined to create this image of the dusty remains of a collapsed star.
- Related Links:
-- Ashes to Ashes, Dust to Dust
-- Tour of G54.1+0.3
The Crab Nebula in 60 Seconds
In 1054 A.D., a star's death in the constellation Taurus was observed on Earth. Now, almost a thousand years later, a superdense neutron star left behind by the explosion is spewing out a blizzard of extremely high-energy particles into the expanding debris field known as the Crab Nebula.
- Related Links:
-- Featured Image Tours
-- Crab Nebula
In 1054 A.D., a star's death in the constellation Taurus was observed on Earth. Now, almost a thousand years later, a superdense neutron star left behind by the explosion is spewing out a blizzard of extremely high-energy particles into the expanding debris field known as the Crab Nebula.
- Related Links:
-- Featured Image Tours
-- Crab Nebula
The Exotic World of Neutron Stars
Neutron stars are created when a massive star runs out of fuel and collapses. As the star collapses, the density becomes so immense that protons and electrons are squeezed tightly together to form neutrons. The end result is a star only 20 km across but weighing 1 1/2 times more than our sun and made up mostly of neutrons.
- Related Links:
-- Neutron Stars/X-ray Binaries
Neutron stars are created when a massive star runs out of fuel and collapses. As the star collapses, the density becomes so immense that protons and electrons are squeezed tightly together to form neutrons. The end result is a star only 20 km across but weighing 1 1/2 times more than our sun and made up mostly of neutrons.
- Related Links:
-- Neutron Stars/X-ray Binaries
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