| Display title | Astronomy:Mars ocean hypothesis |
| Default sort key | Mars ocean hypothesis |
| Page length (in bytes) | 41,124 |
| Namespace ID | 3024 |
| Namespace | Astronomy |
| Page ID | 602920 |
| 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>Steve Marsio |
| Date of page creation | 13:05, 8 February 2024 |
| Latest editor | imported>Steve Marsio |
| Date of latest edit | 13:05, 8 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. | The Mars ocean hypothesis states that nearly a third of the surface of Mars was covered by an ocean of liquid water early in the planet's geologic history. This primordial ocean, dubbed Paleo-Ocean and Oceanus Borealis , would have filled the basin Vastitas Borealis in the northern hemisphere, a region... |
