| Display title | Astronomy:2010 WG9 |
| Default sort key | 2010 WG9 |
| Page length (in bytes) | 8,000 |
| Namespace ID | 3024 |
| Namespace | Astronomy |
| Page ID | 40014 |
| 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>WikiG |
| Date of page creation | 05:57, 18 May 2022 |
| Latest editor | imported>WikiG |
| Date of latest edit | 05:57, 18 May 2022 |
| 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. | 2010 WG9 is a high inclination trans-Neptunian object and slow rotator from the outer Solar System, approximately 100 kilometers in diameter. It was first observed at ESO's La Silla Observatory in northern Chile on 30 November 2010. |
