| Display title | Physics:Molecules in stars |
| Default sort key | Molecules in stars |
| Page length (in bytes) | 16,694 |
| Namespace ID | 3020 |
| Namespace | Physics |
| Page ID | 656993 |
| 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>Corlink |
| Date of page creation | 04:59, 5 February 2024 |
| Latest editor | imported>Corlink |
| Date of latest edit | 04:59, 5 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. | Stellar molecules are molecules that exist or form in stars. Such formations can take place when the temperature is low enough for molecules to form – typically around 6000 K or cooler. Otherwise the stellar matter is restricted to atoms and ions in the forms of gas or – at very high temperatures... |
