Display title | Astronomy:Pair-instability supernova |
Default sort key | Pair-instability supernova |
Page length (in bytes) | 18,330 |
Namespace ID | 3024 |
Namespace | Astronomy |
Page ID | 467947 |
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) |
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Page creator | imported>John Marlo |
Date of page creation | 07:39, 6 February 2024 |
Latest editor | imported>John Marlo |
Date of latest edit | 07:39, 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. | A pair-instability supernova is a type of supernova predicted to occur when pair production, the production of free electrons and positrons in the collision between atomic nuclei and energetic gamma rays, temporarily reduces the internal radiation pressure supporting a supermassive star's core against... |