| Display title | Physics:S-process |
| Default sort key | S-process |
| Page length (in bytes) | 22,509 |
| Namespace ID | 3020 |
| Namespace | Physics |
| Page ID | 648551 |
| 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>Dennis Ross |
| Date of page creation | 15:53, 18 April 2022 |
| Latest editor | imported>Dennis Ross |
| Date of latest edit | 15:53, 18 April 2022 |
| 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 slow neutron-capture process, or s-process, is a series of reactions in nuclear astrophysics that occur in stars, particularly asymptotic giant branch stars. The s-process is responsible for the creation (nucleosynthesis) of approximately half the atomic nuclei heavier than iron.
In the s-process... |
