| Display title | Astronomy:Dark slope streak |
| Default sort key | Dark slope streak |
| Page length (in bytes) | 38,514 |
| Namespace ID | 3024 |
| Namespace | Astronomy |
| Page ID | 638819 |
| 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>OrgMain |
| Date of page creation | 06:51, 6 February 2024 |
| Latest editor | imported>OrgMain |
| Date of latest edit | 06:51, 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. | Dark slope streaks are narrow, avalanche-like features common on dust-covered slopes in the equatorial regions of Mars. They form in relatively steep terrain, such as along escarpments and crater walls. Although first recognized in Viking Orbiter images from the late 1970s, dark slope streaks were not... |
