| Display title | Debris from Martian geysers extend 'flow-like features' - with potential for habitable brines in polar regions |
| Redirects to | Potential for habitable brines flowing from dune spots caused by Martian geysers (info) |
| Default sort key | Debris from Martian geysers extend 'flow-like features' - with potential for habitable brines in polar regions |
| Page length (in bytes) | 94 |
| Namespace ID | 0 |
| Page ID | 4223 |
| Page content language | en - English |
| Page content model | wikitext |
| Indexing by robots | Allowed |
| Number of redirects to this page | 1 |
| Number of subpages of this page | 0 (0 redirects; 0 non-redirects) |
| Delete | Allow all users (infinite) |
| Edit | Allow all users (infinite) |
| Move | Allow all users (infinite) |
| Page creator | Robertinventor (talk | contribs) |
| Date of page creation | 17:58, 25 September 2018 |
| Latest editor | Robertinventor (talk | contribs) |
| Date of latest edit | 17:58, 25 September 2018 |
| Total number of edits | 1 |
| Recent number of edits (within past 180 days) | 0 |
| Recent number of distinct authors | 0 |
