| Display title | Astronomy:Canes II Group |
| Default sort key | Canes II Group |
| Page length (in bytes) | 4,524 |
| Namespace ID | 3024 |
| Namespace | Astronomy |
| Page ID | 374081 |
| 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 |
| HandWiki item ID | None |
| Edit | Allow all users (infinite) |
| Move | Allow all users (infinite) |
| Page creator | imported>Wincert |
| Date of page creation | 12:11, 6 February 2024 |
| Latest editor | imported>Wincert |
| Date of latest edit | 12:11, 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. | The Canes II Group or Canes Venatici II Group (CVn II Group) is a group of galaxies about 26.1 million light-years away from Earth. The group resides in the Local Supercluster. The largest galaxy within the cluster is M106 (NGC 4258), which is a barred spiral galaxy. |
