| Display title | Physics:Supernova nucleosynthesis |
| Default sort key | Supernova Nucleosynthesis |
| Page length (in bytes) | 43,727 |
| Namespace ID | 3020 |
| Namespace | Physics |
| Page ID | 650253 |
| Page content language | en - English |
| Page content model | wikitext |
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| Page creator | imported>Scavis |
| Date of page creation | 04:22, 5 February 2024 |
| Latest editor | imported>Scavis |
| Date of latest edit | 04:22, 5 February 2024 |
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Description | Content |
Article description: (description)
This attribute controls the content of the description and og:description elements. | Supernova nucleosynthesis is the nucleosynthesis of chemical elements in supernova explosions.
In sufficiently massive stars, the nucleosynthesis by fusion of lighter elements into heavier ones occurs during sequential hydrostatic burning processes called helium burning, carbon burning, oxygen burning... |
