chandra_169 September 6th, 2001
Credit: NASA/CXC/SAO/S.Murray et al.
When astronomers used Chandra to observe the remains of a supernova believed to have been observed in 1181 AD, they discovered one of the youngest pulsars known. Embedded in a cloud of high-energy particles, the pulsar is rotating about 15 times a second and is slowing down at the rate of several microseconds per year. A comparison of the rate at which the pulsar is slowing down and its age indicates that the 3C58 pulsar is rotating just about as fast now as when it was formed. This is in contrast to the Crab pulsar, which was formed spinning much more rapidly and has slowed to about half its initial speed.
Provider: Chandra X-ray Observatory
Image Source: http://chandra.harvard.edu/photo/2001/0022/
Curator: Chandra X-ray Observatory, Cambridge, MA, USA
Image Use Policy: http://chandra.harvard.edu/photo/image_use.html
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