| Display title | Astronomy:O-type star |
| Default sort key | O-type star |
| Page length (in bytes) | 32,858 |
| Namespace ID | 3024 |
| Namespace | Astronomy |
| Page ID | 376268 |
| 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 |
| Page image |  |
| HandWiki item ID | None |
| Edit | Allow all users (infinite) |
| Move | Allow all users (infinite) |
| Page creator | imported>LinuxGuru |
| Date of page creation | 12:18, 6 February 2024 |
| Latest editor | imported>LinuxGuru |
| Date of latest edit | 12:18, 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. | An O-type star is a hot, blue-white star of spectral type O in the Yerkes classification system employed by astronomers. They have temperatures in excess of 30,000 kelvins (K). Stars of this type have strong absorption lines of ionised helium, strong lines of other ionised elements, and hydrogen... |
