| Display title | Astronomy:HD 219134 c |
| Default sort key | HD 219134 c |
| Page length (in bytes) | 8,375 |
| Namespace ID | 3024 |
| Namespace | Astronomy |
| Page ID | 18516 |
| 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>WikiGary |
| Date of page creation | 11:46, 6 February 2024 |
| Latest editor | imported>WikiGary |
| Date of latest edit | 11:46, 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. | HD 219134 c, also known as HR 8832 c, is a hot, dense, rocky exoplanet orbiting around the K-type star HD 219134 in the constellation of Cassiopeia. Originally thought to be a little less than three times the mass of Earth, it is now known to be over 4 times the mass and 51% larger in radius, suggesting... |
