| Display title | Astronomy:Carbon-burning process |
| Default sort key | Carbon-burning process |
| Page length (in bytes) | 15,513 |
| Namespace ID | 3024 |
| Namespace | Astronomy |
| Page ID | 374107 |
| 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 |
| HandWiki item ID | None |
| Edit | Allow all users (infinite) |
| Move | Allow all users (infinite) |
| Page creator | imported>OrgMain |
| Date of page creation | 13:58, 26 September 2021 |
| Latest editor | imported>OrgMain |
| Date of latest edit | 13:58, 26 September 2021 |
| 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 carbon-burning process or carbon fusion is a set of nuclear fusion reactions that take place in the cores of massive stars (at least 8 $ {\begin{smallmatrix}M\odot \end{smallmatrix}} $ at birth) that combines carbon into other elements. It requires high temperatures (> 5×108 K or 50 keV) and densities... |
