| Display title | Astronomy:Protoplanetary disk |
| Default sort key | Protoplanetary disk |
| Page length (in bytes) | 21,943 |
| Namespace ID | 3024 |
| Namespace | Astronomy |
| Page ID | 576597 |
| 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>CodeMe |
| Date of page creation | 09:06, 6 February 2024 |
| Latest editor | imported>CodeMe |
| Date of latest edit | 09:06, 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. | A protoplanetary disk is a rotating circumstellar disc of dense gas and dust surrounding a young newly formed star, a T Tauri star, or Herbig Ae/Be star. The protoplanetary disk may also be considered an accretion disk for the star itself, because gases or other material may be falling from the inner... |
