| Display title | Physics:Geometric albedo |
| Default sort key | Geometric Albedo |
| Page length (in bytes) | 11,632 |
| Namespace ID | 3020 |
| Namespace | Physics |
| Page ID | 652909 |
| Page content language | en - English |
| Page content model | wikitext |
| Indexing by robots | Allowed |
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| Counted as a content page | Yes |
| HandWiki item ID | None |
| Edit | Allow all users (infinite) |
| Move | Allow all users (infinite) |
| Page creator | imported>Nautica |
| Date of page creation | 23:55, 5 March 2023 |
| Latest editor | imported>Nautica |
| Date of latest edit | 23:55, 5 March 2023 |
| 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. | In astronomy, the geometric albedo of a celestial body is the ratio of its actual brightness as seen from the light source (i.e. at zero phase angle) to that of an idealized flat, fully reflecting, diffusively scattering (Lambertian) disk with the same cross-section. (This phase angle refers to the direction... |
