| Display title | Physics:Bond albedo |
| Default sort key | Bond albedo |
| Page length (in bytes) | 9,365 |
| Namespace ID | 3020 |
| Namespace | Physics |
| Page ID | 653816 |
| 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>Gametune |
| Date of page creation | 19:43, 25 June 2023 |
| Latest editor | imported>Gametune |
| Date of latest edit | 19:43, 25 June 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. | The Bond albedo (also called spheric albedo, planetary albedo, and bolometric albedo), named after the American astronomer George Phillips Bond (1825–1865), who originally proposed it, is the fraction of power in the total electromagnetic radiation incident on an astronomical body that is scattered back... |
