| Display title | Astronomy:Outflow channels |
| Default sort key | Outflow channels |
| Page length (in bytes) | 12,856 |
| Namespace ID | 3024 |
| Namespace | Astronomy |
| Page ID | 25947 |
| 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>John Marlo |
| Date of page creation | 13:47, 6 February 2024 |
| Latest editor | imported>John Marlo |
| Date of latest edit | 13:47, 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. | Outflow channels are extremely long, wide swathes of scoured ground on Mars. They extend many hundreds of kilometers in length and are typically greater than one kilometer in width. They are thought to have been carved by huge outburst floods.
Crater counts indicate that most of the channels were cut... |
