| Display title | Astronomy:WASP-75 |
| Default sort key | WASP-75 |
| Page length (in bytes) | 5,852 |
| Namespace ID | 3024 |
| Namespace | Astronomy |
| Page ID | 36996 |
| 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>Raymond Straus |
| Date of page creation | 11:53, 8 February 2024 |
| Latest editor | imported>Raymond Straus |
| Date of latest edit | 11:53, 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. | WASP-75 is a F-type main-sequence star about 980 light-years away. The star is much younger than the Sun at approximately 2.9±0.2 billion years. WASP-75 is similar to the Sun in its concentration of heavy elements. |
