Display title | Astronomy:Standard solar model |
Default sort key | Standard solar model |
Page length (in bytes) | 29,803 |
Namespace ID | 3024 |
Namespace | Astronomy |
Page ID | 377493 |
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>S.Timg |
Date of page creation | 07:11, 6 February 2024 |
Latest editor | imported>S.Timg |
Date of latest edit | 07:11, 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 standard solar model (SSM) is a mathematical treatment of the Sun as a spherical ball of gas (in varying states of ionisation, with the hydrogen in the deep interior being a completely ionised plasma). This model, technically the spherically symmetric quasi-static model of a star, has stellar structure... |