| Display title | Astronomy:Tau Draconis |
| Default sort key | Tau Draconis |
| Page length (in bytes) | 7,380 |
| Namespace ID | 3024 |
| Namespace | Astronomy |
| Page ID | 480504 |
| 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>DanMescoff |
| Date of page creation | 10:49, 8 February 2024 |
| Latest editor | imported>DanMescoff |
| Date of latest edit | 10:49, 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. | Tau Draconis, Latinized from τ Draconis, is an astrometric binary star system in the northern circumpolar constellation of Draco. The star is faintly visible to the naked eye, having an apparent visual magnitude of 4.45. Based upon an annual parallax shift of 22.28 mas as measured from Earth, it... |
