Crab Pulsar
Use attributes for filter ! | |
Mass | 2. 784 × 10^30 kg (1. 4 M☉) |
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Radius | 10 km |
Surface temperature | 1. 6 million K |
Age | 965 years |
Luminosity | 0. 9 L☉ |
B−V color index | +0. 5 |
Date of Reg. | |
Date of Upd. | |
ID | 2341578 |
About Crab Pulsar
The Crab Pulsar is a relatively young neutron star. The star is the central star in the Crab Nebula, a remnant of the supernova SN 1054, which was widely observed on Earth in the year 1054. Discovered in 1968, the pulsar was the first to be connected with a supernova remnant.