| Display title | Astronomy:Iota Octantis |
| Default sort key | Iota Octantis |
| Page length (in bytes) | 9,015 |
| Namespace ID | 3024 |
| Namespace | Astronomy |
| Page ID | 838457 |
| 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>AnLinks |
| Date of page creation | 15:00, 8 February 2024 |
| Latest editor | imported>AnLinks |
| Date of latest edit | 15:00, 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. | Iota Octantis, Latinized, from ι Octantis is a double star in the southern circumpolar constellation Octans. The "A" component has an apparent magnitude of 5.83, making it faintly visible to the naked eye under ideal conditions, but the "B" component can't be seen due to its faintness. The system is... |
