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- Q2832068 subject Q6306516.
- Q2832068 subject Q6375730.
- Q2832068 subject Q8706947.
- Q2832068 abstract "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. (Note that this phase angle refers to the direction of the light paths and is not a phase angle in its normal meaning in optics or electronics.)Diffuse scattering implies that radiation is reflected isotropically with no memory of the location of the incident light source. Zero phase angle corresponds to looking along the direction of illumination. For Earth-bound observers this occurs when the body in question is at opposition and on the ecliptic.The visual geometric albedo refers to the geometric albedo quantity when accounting for only electromagnetic radiation in the visible spectrum.".
- Q2832068 wikiPageExternalLink ?glossary&term=albedo.
- Q2832068 wikiPageWikiLink Q101038.
- Q2832068 wikiPageWikiLink Q105562.
- Q2832068 wikiPageWikiLink Q1057392.
- Q2832068 wikiPageWikiLink Q106551.
- Q2832068 wikiPageWikiLink Q11386.
- Q2832068 wikiPageWikiLink Q1154504.
- Q2832068 wikiPageWikiLink Q15047.
- Q2832068 wikiPageWikiLink Q185553.
- Q2832068 wikiPageWikiLink Q193.
- Q2832068 wikiPageWikiLink Q2027206.
- Q2832068 wikiPageWikiLink Q205034.
- Q2832068 wikiPageWikiLink Q2059855.
- Q2832068 wikiPageWikiLink Q2731139.
- Q2832068 wikiPageWikiLink Q3303.
- Q2832068 wikiPageWikiLink Q333.
- Q2832068 wikiPageWikiLink Q466686.
- Q2832068 wikiPageWikiLink Q507546.
- Q2832068 wikiPageWikiLink Q544.
- Q2832068 wikiPageWikiLink Q5651619.
- Q2832068 wikiPageWikiLink Q6306516.
- Q2832068 wikiPageWikiLink Q6375730.
- Q2832068 wikiPageWikiLink Q6999.
- Q2832068 wikiPageWikiLink Q76299.
- Q2832068 wikiPageWikiLink Q79852.
- Q2832068 wikiPageWikiLink Q827674.
- Q2832068 wikiPageWikiLink Q856980.
- Q2832068 wikiPageWikiLink Q8706947.
- Q2832068 comment "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.".
- Q2832068 label "Geometric albedo".