Difference between revisions of "Template:Astronomical albedo table"
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blackwiki>Planet photometry (Updated several planetary albedos. Provided citations for original journal articles, where known, in place of 'NASA Fact Sheets' which do not specifically cite the sources of their data values.) |
blackwiki>Trappist the monk m (cite repair;) |
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| − | |[[Venus]] <ref name="Haus_et_al">{{cite journal |title=Radiative energy balance of Venus based on improved models of the middle and lower atmosphere |journal=Icarus |first1=R. |last1=Haus | + | |[[Venus]] <ref name="Haus_et_al">{{cite journal |title=Radiative energy balance of Venus based on improved models of the middle and lower atmosphere |journal=Icarus |first1=R. |last1=Haus |display-authors=etal |volume=272 |pages=178-205 |date=July 2016 |doi=10.1016/j.icarus.2016.02.048 |bibcode=2016Icar..272..178H }}</ref> <ref name="Mallama_et_al"/> |
|{{bartable|0.76||100}} | |{{bartable|0.76||100}} | ||
|{{bartable|0.689||100}} | |{{bartable|0.689||100}} | ||
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|{{bartable|0.17||100}} | |{{bartable|0.17||100}} | ||
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| − | |[[Jupiter]] <ref name="Li_et_al">{{cite journal |title=Less absorbed solar energy and more internal heat for Jupiter |first1=Liming |last1=Li | + | |[[Jupiter]] <ref name="Li_et_al">{{cite journal |title=Less absorbed solar energy and more internal heat for Jupiter |first1=Liming |last1=Li |display-authors=etal |journal=Nature Communications |date=2018 |doi=10.1038/s41467-018-06107-2 }}</ref> <ref name="Mallama_et_al"/> |
|{{bartable|0.503||100}} | |{{bartable|0.503||100}} | ||
|{{bartable|0.538||100}} | |{{bartable|0.538||100}} | ||
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| − | |[[Saturn]] <ref name="Hanel_et_al">{{cite journal |title=Albedo, internal heat flux, and energy balance of Saturn |first1=R.A. |last1=Hanel | + | |[[Saturn]] <ref name="Hanel_et_al">{{cite journal |title=Albedo, internal heat flux, and energy balance of Saturn |first1=R.A. |last1=Hanel |display-authors=etal |journal=Icarus |volume=53 |pages=262 |date=1983 |doi=10.1016/0019-1035(83)90147-1 |bibcode=1983Icar...53..262H }}</ref> <ref name="Mallama_et_al"/> |
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|{{bartable|1.4||100}} | |{{bartable|1.4||100}} | ||
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| − | |[[Uranus]] <ref name="Pearl_et_al_Uranus">{{cite journal |title=The albedo, effective temperature, and energy balance of Uranus, as determined from Voyager IRIS data |first1=J.C. |last1=Pearl | + | |[[Uranus]] <ref name="Pearl_et_al_Uranus">{{cite journal |title=The albedo, effective temperature, and energy balance of Uranus, as determined from Voyager IRIS data |first1=J.C. |last1=Pearl |display-authors=etal |journal=Icarus |volume=84 |pages=12-28 |date=1990 |doi=10.1016/0019-1035(90)90155-3 |bibcode=1990Icar...84...12P }}</ref> <ref name="Mallama_et_al"/> |
|{{bartable|0.300||100}} | |{{bartable|0.300||100}} | ||
|{{bartable|0.488||100}} | |{{bartable|0.488||100}} | ||
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| − | |[[Neptune]] <ref name="Pearl_et_al_Neptune">{{cite journal |title=The albedo, effective temperature, and energy balance of Neptune, as determined from Voyager data |first1=J.C. |last1=Pearl | + | |[[Neptune]] <ref name="Pearl_et_al_Neptune">{{cite journal |title=The albedo, effective temperature, and energy balance of Neptune, as determined from Voyager data |first1=J.C. |last1=Pearl |display-authors=etal |journal=J. Geophys. Res. |volume=96 |pages=18,921-18,930 |date=1991 |doi=10.1029/91JA01087 |bibcode=1991JGR....9618921P }}</ref> <ref name="Mallama_et_al"/> |
|{{bartable|0.290||100}} | |{{bartable|0.290||100}} | ||
|{{bartable|0.442||100}} | |{{bartable|0.442||100}} | ||
Revision as of 22:23, 8 February 2019
Name Bond albedo Visual geometric albedo Mercury [1] [2] 0.088 0.142 Venus [3] [2] 0.76 0.689 Earth [4] [2] 0.306 0.434 Moon[5] [5] 0.11 0.12 Mars [6] [2] 0.25 0.17 Jupiter [7] [2] 0.503 0.538 Saturn [8] [2] 0.342 0.499 Enceladus[9] 0.8 1.4 Uranus [10] [2] 0.300 0.488 Neptune [11] [2] 0.290 0.442 Pluto 0.4 0.44–0.61 Eris 0.96 —
References
- ↑ Mallama, Anthony (2017). "The spherical bolometric albedo for planet Mercury". arXiv:1703.02670. Cite journal requires
|journal=(help) - ↑ 2.0 2.1 2.2 2.3 2.4 2.5 2.6 2.7 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. Bibcode:2017Icar..282...19M. doi:10.1016/j.icarus.2016.09.023.
- ↑ Haus, R.; et al. (July 2016). "Radiative energy balance of Venus based on improved models of the middle and lower atmosphere". Icarus. 272: 178–205. Bibcode:2016Icar..272..178H. doi:10.1016/j.icarus.2016.02.048.
- ↑ Williams, David R. (2004-09-01). "Earth Fact Sheet". NASA. Retrieved 2010-08-09.
- ↑ 5.0 5.1 Williams, David R. (2014-04-25). "Moon Fact Sheet". NASA. Retrieved 2015-03-02.
- ↑ Mars Fact Sheet, NASA
- ↑ Li, Liming; et al. (2018). "Less absorbed solar energy and more internal heat for Jupiter". Nature Communications. doi:10.1038/s41467-018-06107-2.
- ↑ Hanel, R.A.; et al. (1983). "Albedo, internal heat flux, and energy balance of Saturn". Icarus. 53: 262. Bibcode:1983Icar...53..262H. doi:10.1016/0019-1035(83)90147-1.
- ↑ See the discussion here for explanation of this unusual value above one.
- ↑ Pearl, J.C.; et al. (1990). "The albedo, effective temperature, and energy balance of Uranus, as determined from Voyager IRIS data". Icarus. 84: 12–28. Bibcode:1990Icar...84...12P. doi:10.1016/0019-1035(90)90155-3.
- ↑ Pearl, J.C.; et al. (1991). "The albedo, effective temperature, and energy balance of Neptune, as determined from Voyager data". J. Geophys. Res. 96: 18, 921–18, 930. Bibcode:1991JGR....9618921P. doi:10.1029/91JA01087.