| Display title | Astronomy:YBP 1194 |
| Default sort key | YBP 1194 |
| Page length (in bytes) | 8,608 |
| Namespace ID | 3024 |
| Namespace | Astronomy |
| Page ID | 180597 |
| Page content language | en - English |
| Page content model | wikitext |
| Indexing by robots | Allowed |
| Number of redirects to this page | 1 |
| Counted as a content page | Yes |
| HandWiki item ID | None |
| Edit | Allow all users (infinite) |
| Move | Allow all users (infinite) |
| Page creator | imported>StanislovAI |
| Date of page creation | 14:01, 14 February 2024 |
| Latest editor | imported>StanislovAI |
| Date of latest edit | 14:01, 14 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. | YBP 1194 is a G-type main-sequence star, class G5V, in the open cluster M67 in the constellation Cancer. It is the best solar twin found to date, having the near exact temperature and mass as the Sun. YBP 1194 has a higher metallicity than the Sun and is 0.5 billion years younger at an age of 4.2 billion... |
