| Display title | Astronomy:Dao Vallis |
| Default sort key | Dao Vallis |
| Page length (in bytes) | 3,141 |
| Namespace ID | 3024 |
| Namespace | Astronomy |
| Page ID | 19263 |
| 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>StanislovAI |
| Date of page creation | 13:30, 26 September 2021 |
| Latest editor | imported>StanislovAI |
| Date of latest edit | 13:30, 26 September 2021 |
| 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. | Dao Vallis is a valley on Mars that appears to have been carved by water. It runs southwestward into Hellas Planitia from the southern slopes of the volcano Hadriacus Mons, and has been identified as an outflow channel. It and its tributary, Niger Vallis, extend for about 1,200 km (750 mi) |
