Physics:Bond albedo
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 out into space.
Because the Bond albedo accounts for all of the light scattered from a body at all wavelengths and all phase angles, it is a necessary quantity for determining how much energy a body absorbs. This, in turn, is crucial for determining the equilibrium temperature of a body.
Because bodies in the outer Solar System are always observed at very low phase angles from the Earth, the only reliable data for measuring their Bond albedo comes from spacecraft.
Phase integral
The Bond albedo (A) is related to the geometric albedo (p) by the expression
- [math]\displaystyle{ A = pq }[/math]
where q is termed the phase integral and is given in terms of the directional scattered flux I(α) into phase angle α (averaged over all wavelengths and azimuthal angles) as
- [math]\displaystyle{ q = 2\int_0^\pi \frac{I(\alpha)}{I(0)} \sin\alpha \, d\alpha. }[/math]
The phase angle α is the angle between the source of the radiation (usually the Sun) and the observing direction, and varies from zero for light scattered back towards the source, to 180° for observations looking towards the source. For example, during opposition or looking at the full moon, α is very small, while backlit objects or the new moon have α close to 180°.
Examples
The Bond albedo is a value strictly between 0 and 1, as it includes all possible scattered light (but not radiation from the body itself). This is in contrast to other definitions of albedo such as the geometric albedo, which can be above 1. In general, though, the Bond albedo may be greater or smaller than the geometric albedo, depending on the surface and atmospheric properties of the body in question.
Some examples:[1]
| Name | Bond albedo | Visual geometric albedo | ||
|---|---|---|---|---|
| Mercury[2][3] | 0.088 | 0.142 | ||
| Venus[4][3] | 0.76 | 0.689 | ||
| Earth[5][3] | 0.306 | 0.434 | ||
| Moon[6] | 0.11 | 0.12 | ||
| Mars [7][3] | 0.25 | 0.17 | ||
| Jupiter[8][3] | 0.503 | 0.538 | ||
| Saturn[9][3] | 0.342 | 0.499 | ||
| Enceladus[10][11] | 0.81 | 1.375 | ||
| Uranus[12][3] | 0.300 | 0.488 | ||
| Neptune[13][3] | 0.290 | 0.442 | ||
| Pluto[14] | 0.41 | 0.51 | ||
| Charon[15] | 0.29 | 0.41 | ||
| Haumea[14] | 0.33 | 0.66 | ||
| Makemake[14] | 0.74 | 0.82 | ||
| Eris[14] | 0.99 | 0.96 | ||
See also
References
- ↑ Albedo of the Earth
- ↑ Mallama, Anthony (2017). "The spherical bolometric albedo for planet Mercury". arXiv:1703.02670 [astro-ph.EP].
- ↑ 3.0 3.1 3.2 3.3 3.4 3.5 3.6 3.7 Mallama, Anthony; Krobusek, Bruce; Pavlov, Hristo (2017). "Comprehensive wide-band magnitudes and albedos for the planets, with applications to exo-planets and Planet Nine". Icarus 282: 19–33. doi:10.1016/j.icarus.2016.09.023. Bibcode: 2017Icar..282...19M.
- ↑ Haus, R. (July 2016). "Radiative energy balance of Venus based on improved models of the middle and lower atmosphere". Icarus 272: 178–205. doi:10.1016/j.icarus.2016.02.048. Bibcode: 2016Icar..272..178H. https://elib.dlr.de/107059/1/haus_improved_energybalance_icarus_2016_preprint.pdf.
- ↑ Williams, David R. (2004-09-01). "Earth Fact Sheet". NASA. http://nssdc.gsfc.nasa.gov/planetary/factsheet/earthfact.html.
- ↑ Williams, David R. (2014-04-25). "Moon Fact Sheet". NASA. http://nssdc.gsfc.nasa.gov/planetary/factsheet/moonfact.html.
- ↑ Mars Fact Sheet, NASA
- ↑ Li, Liming (2018). "Less absorbed solar energy and more internal heat for Jupiter". Nature Communications 9 (1): 3709. doi:10.1038/s41467-018-06107-2. PMID 30213944. Bibcode: 2018NatCo...9.3709L.
- ↑ Hanel, R.A. (1983). "Albedo, internal heat flux, and energy balance of Saturn". Icarus 53 (2): 262–285. doi:10.1016/0019-1035(83)90147-1. Bibcode: 1983Icar...53..262H.
- ↑ Verbiscer, A.; French, R.; Showalter, M.; Helfenstein, P. (February 9, 2007). "Enceladus: Cosmic Graffiti Artist Caught in the Act". Science 315 (5813): 815. doi:10.1126/science.1134681. PMID 17289992. Bibcode: 2007Sci...315..815V. (supporting online material, table S1)
- ↑ Howett, Carly J. A.; Spencer, John R.; Pearl, J. C.; Segura, M. (2010). "Thermal inertia and bolometric Bond albedo values for Mimas, Enceladus, Tethys, Dione, Rhea and Iapetus as derived from Cassini/CIRS measurements". Icarus 206 (2): 573–593. doi:10.1016/j.icarus.2009.07.016. Bibcode: 2010Icar..206..573H.
- ↑ Pearl, J.C. (1990). "The albedo, effective temperature, and energy balance of Uranus, as determined from Voyager IRIS data". Icarus 84 (1): 12–28. doi:10.1016/0019-1035(90)90155-3. Bibcode: 1990Icar...84...12P.
- ↑ Pearl, J.C. (1991). "The albedo, effective temperature, and energy balance of Neptune, as determined from Voyager data". J. Geophys. Res. 96: 18,921-18,930. doi:10.1029/91JA01087. Bibcode: 1991JGR....9618921P.
- ↑ 14.0 14.1 14.2 14.3 Verbiscer, Anne J.Expression error: Unrecognized word "etal". (April 2022). "The Diverse Shapes of Dwarf Planet and Large KBO Phase Curves Observed from New Horizons". The Planetary Science Journal 3 (4): 31. doi:10.3847/PSJ/ac63a6. 95. Bibcode: 2022PSJ.....3...95V.
- ↑ Buratti, B. J.; Hicks, M. D.; Hillier, J. H.; Verbiscer, A. J.; Abgarian, M.; Hofgartner, J. D.; Lauer, T. R.; Grundy, W. M. et al. (2019-03-19). "New Horizons Photometry of Pluto's Moon Charon". The Astrophysical Journal 874 (1): L3. doi:10.3847/2041-8213/ab0bff. ISSN 2041-8213. Bibcode: 2019ApJ...874L...3B.
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