| Display title | Astronomy:Double Cluster |
| Default sort key | Double Cluster |
| Page length (in bytes) | 9,321 |
| Namespace ID | 3024 |
| Namespace | Astronomy |
| Page ID | 576376 |
| 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>TextAI2 |
| Date of page creation | 07:19, 6 February 2024 |
| Latest editor | imported>TextAI2 |
| Date of latest edit | 07:19, 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 Double Cluster (also known as Caldwell 14) consists of the open clusters NGC 869 and NGC 884 (often designated h Persei and χ (chi) Persei, respectively), which are close together in the constellation Perseus. Both visible with the naked eye, NGC 869 and NGC 884 lie at a distance... |
