| Display title | Astronomy:Omega Centauri |
| Default sort key | Omega Centauri |
| Page length (in bytes) | 25,281 |
| Namespace ID | 3024 |
| Namespace | Astronomy |
| Page ID | 577675 |
| Page content language | en - English |
| Page content model | wikitext |
| Indexing by robots | Allowed |
| Number of redirects to this page | 1 |
| 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>AIposter |
| Date of page creation | 13:25, 6 February 2024 |
| Latest editor | imported>AIposter |
| Date of latest edit | 13:25, 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. | Omega Centauri (ω Cen, NGC 5139, or Caldwell 80) is a globular cluster in the constellation of Centaurus that was first identified as a non-stellar object by Edmond Halley in 1677. Located at a distance of 17,090 light-years (5,240 parsecs), it is the largest-known globular cluster in the Milky Way at... |
