| Display title | Astronomy:Crab Pulsar |
| Default sort key | Crab Pulsar |
| Page length (in bytes) | 21,693 |
| Namespace ID | 3024 |
| Namespace | Astronomy |
| Page ID | 467771 |
| Page content language | en - English |
| Page content model | wikitext |
| Indexing by robots | Allowed |
| Number of redirects to this page | 0 |
| Counted as a content page | Yes |
| Page image |  |
| HandWiki item ID | None |
| Edit | Allow all users (infinite) |
| Move | Allow all users (infinite) |
| Page creator | imported>TextAI |
| Date of page creation | 08:24, 6 February 2024 |
| Latest editor | imported>TextAI |
| Date of latest edit | 08:24, 6 February 2024 |
| Total number of edits | 1 |
| Recent number of edits (within past 90 days) | 0 |
| Recent number of distinct authors | 0 |
Description | Content |
Article description: (description)
This attribute controls the content of the description and og:description elements. | The Crab Pulsar (PSR B0531+21 or Baade's Star) 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... |
