| Display title | Astronomy:Mu Arae |
| Default sort key | Mu Arae |
| Page length (in bytes) | 27,236 |
| Namespace ID | 3024 |
| Namespace | Astronomy |
| Page ID | 575707 |
| 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>Scavis2 |
| Date of page creation | 11:56, 8 February 2024 |
| Latest editor | imported>Scavis2 |
| Date of latest edit | 11:56, 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. | Mu Arae (μ Arae, abbreviated Mu Ara, μ Ara), often designated HD 160691, officially named Cervantes sur-VAN-teez, is a main sequence G-type star approximately 50 light-years away from the Sun in the constellation of Ara. The star has a planetary system with four known extrasolar planets (designated... |
