| Display title | Astronomy:Schwarzschild criterion |
| Default sort key | Schwarzschild criterion |
| Page length (in bytes) | 2,388 |
| Namespace ID | 3024 |
| Namespace | Astronomy |
| Page ID | 377052 |
| 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>John Stpola |
| Date of page creation | 10:27, 6 February 2024 |
| Latest editor | imported>John Stpola |
| Date of latest edit | 10:27, 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. | Discovered by Karl Schwarzschild, the Schwarzschild criterion is a criterion in astrophysics where a stellar medium is stable against convection when the rate of change in temperature (T) by altitude (Z) satisfies
$ -{\frac {dT}{dZ}}<{\frac {g}{C_{p}}} $
where $ g $ is gravity and $ C_{p} $ is the... |
