| Display title | Astronomy:Mare Anguis |
| Default sort key | Mare Anguis |
| Page length (in bytes) | 3,530 |
| Namespace ID | 3024 |
| Namespace | Astronomy |
| Page ID | 944928 |
| 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>DanMescoff |
| Date of page creation | 13:24, 14 February 2024 |
| Latest editor | imported>DanMescoff |
| Date of latest edit | 13:24, 14 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. | Mare Anguis (Latin anguis, the "serpent sea") is a lunar mare located on the near side of the Moon, about 150 kilometers in diameter. Located within the Crisium basin, Mare Anguis is a part of the Nectarian System, meaning that it was formed during the Nectarian time period. Like most mare, the surface... |
