| Display title | Astronomy:Inclination instability |
| Default sort key | Inclination instability |
| Page length (in bytes) | 4,269 |
| Namespace ID | 3024 |
| Namespace | Astronomy |
| Page ID | 617787 |
| 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>LinuxGuru |
| Date of page creation | 14:28, 6 February 2024 |
| Latest editor | imported>LinuxGuru |
| Date of latest edit | 14:28, 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. | An inclination instability is a dynamical instability that can occur in a disk of objects with eccentric orbits, causing it to form into a conical shape. The gravity of the objects causes an exponential growth of their inclinations while reducing their eccentricities. The inclination instability also... |
