| Display title | Astronomy:IC 4499 |
| Default sort key | IC 4499 |
| Page length (in bytes) | 3,569 |
| Namespace ID | 3024 |
| Namespace | Astronomy |
| Page ID | 18553 |
| 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>Dennis Ross |
| Date of page creation | 14:06, 8 February 2024 |
| Latest editor | imported>Dennis Ross |
| Date of latest edit | 14:06, 8 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. | IC 4499 is a loose globular cluster in the constellation Apus. It is located in the medium-far galactic halo. Its apparent magnitude is 9.76, and was thought to be unusual because it appears to be 3–4 billion years younger than most other globular clusters in the Milky Way, as determined by metallicity... |
