| Display title | Astronomy:Dark flow |
| Default sort key | Dark flow |
| Page length (in bytes) | 15,260 |
| Namespace ID | 3024 |
| Namespace | Astronomy |
| Page ID | 374549 |
| 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 | 12:47, 6 February 2024 |
| Latest editor | imported>StanislovAI |
| Date of latest edit | 12:47, 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. | In astrophysics, dark flow is a controversial hypothesis to explain certain non-random measurements of peculiar velocity of galaxy clusters. The actual measured velocity is the sum of the velocity predicted by Hubble's Law plus a possible small velocity flowing in a common direction. Very large scale... |
