| Display title | Astronomy:Owl Nebula |
| Default sort key | Owl Nebula |
| Page length (in bytes) | 16,208 |
| Namespace ID | 3024 |
| Namespace | Astronomy |
| Page ID | 376270 |
| 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 |
| Page image |  |
| HandWiki item ID | None |
| Edit | Allow all users (infinite) |
| Move | Allow all users (infinite) |
| Page creator | imported>JMinHep |
| Date of page creation | 06:06, 6 February 2024 |
| Latest editor | imported>JMinHep |
| Date of latest edit | 06:06, 6 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. | The Owl Nebula (also known as Messier 97, M97 or NGC 3587) is a planetary nebula approximately 2,030 light years away in the constellation Ursa Major. Estimated to be about 8,000 years old, it is approximately circular in cross-section with a faint internal structure. It was formed from the outflow of... |
