| Display title | Astronomy:Grey atmosphere |
| Default sort key | Grey Atmosphere |
| Page length (in bytes) | 9,744 |
| Namespace ID | 3024 |
| Namespace | Astronomy |
| Page ID | 375309 |
| 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>MedAI |
| Date of page creation | 13:31, 6 February 2024 |
| Latest editor | imported>MedAI |
| Date of latest edit | 13:31, 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 Grey atmosphere (or gray) is a useful set of approximations made for radiative transfer applications in studies of stellar atmospheres (atmospheres of stars) based on the simplified notion that the absorption coefficient $ \alpha _{\nu } $ of matter within a star's atmosphere is constant—that is... |
