Crab Pulsar
| Use attributes for filter ! | |
| Mass | 2. 784 × 10^30 kg (1. 4 M☉) |
|---|---|
| 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.