| Display title | Astronomy:Gravitational compression |
| Default sort key | Gravitational compression |
| Page length (in bytes) | 3,725 |
| Namespace ID | 3024 |
| Namespace | Astronomy |
| Page ID | 375274 |
| 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 |
| Page image |  |
| HandWiki item ID | None |
| Edit | Allow all users (infinite) |
| Move | Allow all users (infinite) |
| Page creator | imported>S.Timg |
| Date of page creation | 03:02, 27 June 2023 |
| Latest editor | imported>S.Timg |
| Date of latest edit | 03:02, 27 June 2023 |
| 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. | Gravitational compression is a phenomenon in which gravity, acting on the mass of an object, compresses it, reducing its size and increasing the object's density.
At the center of a planet or star, gravitational compression produces heat by the Kelvin–Helmholtz mechanism. This is the mechanism that... |
