| Display title | Astronomy:Theta1 Orionis B |
| Default sort key | Theta1 Orionis B |
| Page length (in bytes) | 10,054 |
| Namespace ID | 3024 |
| Namespace | Astronomy |
| Page ID | 580445 |
| 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>Scavis |
| Date of page creation | 13:16, 8 February 2024 |
| Latest editor | imported>Scavis |
| Date of latest edit | 13:16, 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. | Theta1 Orionis B (θ1 Orionis B), also known as BM Orionis, is a multiple star system containing at least five members. It is also one of the main stars of the Trapezium Cluster, with the others being A, C, and D. The primary is an eclipsing variable and one of the youngest known eclipsing binary systems... |
