火卫一
参考资料

↑  NASA Celestia 的存檔，存档日期2005-03-09.
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1 2  . DLR. 2008-10-16  [2008-10-16]. （原始内容存档于2011-06-04）.
1 2  按照平均半径11.1千米计算，体积×密度（1.877 g/cm3）= 质量，约为1.07×1016 kg。逃逸速度为11.3m/s（40 km/h）
1 2 3  Andert, T. P.; Rosenblatt, P.; Pätzold, M.; Häusler, B.; Dehant, V.; Tyler, G. L.; Marty, J. C. . Geophysical Research Letters (American Geophysical Union). 2010-05-07, 37 (L09202)  [2010-10-01]. Bibcode:2010GeoRL..3709202A. doi:10.1029/2009GL041829. （原始内容存档于2010-06-26）.  引文使用过时参数coauthors (帮助)
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↑  . The Observatory. 1877-09-20, 1 (6): 181–185  [2009-02-04]. Bibcode:1877Obs.....1..181.. （原始内容存档于2019-05-19）.
↑  Hall, A.  91 (2161). Astronomische Nachrichten: 11/12–13/14. 1877-10-17  [2009-02-04]. （原始内容存档于2019-05-20）.
↑  Morley, T. A. . Astronomy and Astrophysics Supplement Series (ISSN 0365-0138). February 1989, 77 (2): 209–226  [2011-11-07]. （原始内容存档于2018-07-27）.  (Table II, p. 220: first observation of Phobos on August 18, 1877.38498)
↑  Madan, H. G. . Nature (Macmillan Journals ltd.). 1877-10-04, 16 (414): 475. Bibcode:1877Natur..16R.475M. doi:10.1038/016475b0.
↑  Hall, A. . Astronomische Nachrichten. 1878-03-14, 92 (2187): 47–48  [2011-11-07]. Bibcode:1878AN.....92...47H. doi:10.1002/asna.18780920304. （原始内容存档于2011-11-15）.
↑  .   [2011-11-07]. （原始内容存档于2011-11-14）.
↑  Lewis, J. S. . Elsevier Academic Press. 2004: 425. ISBN 0-12-446744-X.
↑  . （原始内容存档于2007-09-26）. When the error bars are taken into account, only one of these, Phobos, has a porosity below 0.2...
↑  .   [2011-11-07]. （原始内容存档于2012-01-14）. It is light, with a density less than twice that of water, and orbits just 5989 km above the Martian surface.
↑  Busch, M. W.; et al.. . Icarus. 2007, 186 (2): 581–584. Bibcode:2007Icar..186..581B. doi:10.1016/j.icarus.2006.11.003.  引文使用过时参数coauthors (帮助)
↑  Murchie, S. L.; Erard, S., Langevin, Y., Britt, D. T., Bibring, J. P., and Mustard, J. F. . Abstracts of the Lunar and Planetary Science Conference. 1991, 22: 943.  引文使用过时参数coauthors (帮助)
↑  Rivkin, A. S.; et al.. . Icarus. 2002年3月, 156 (1): 64. Bibcode:2002Icar..156...64R. doi:10.1006/icar.2001.6767.  引文使用过时参数coauthors (帮助)
↑  Fanale, F. P.; Salvail, J. R. . Geophys. Res. Lett. 1989, 16 (4): 287–290. Bibcode:1989GeoRL..16..287F. doi:10.1029/GL016i004p00287.
↑  Fanale, Fraser P.; Salvail, James R. . Icarus (International Journal of the Solar System) (USA). Dec 1990, 88: 380–395. Bibcode:1990Icar...88..380F. ISSN 0019-1035. doi:10.1016/0019-1035(90)90089-R.
↑  Showalter, M. R.; Hamilton, D. P. and Nicholson, P. D.  (PDF). Planetary and Space Science. 2006, 54 (9-10): 844–854  [2011-11-07]. Bibcode:2006P&SS...54..844S. doi:10.1016/j.pss.2006.05.009. （原始内容存档 (PDF)于2011-06-06）.  引文使用过时参数coauthors (帮助)
↑  Britt, Robert Roy. . space.com. 2001-03-13  [2010-05-12]. （原始内容存档于2010-03-09）.
↑  . （原始内容存档于2007-03-07）.
↑  . New Scientist. 1976-10-21: 158.  使用|accessdate=需要含有|url= (帮助)
↑  .   [2011-11-07]. （原始内容存档于2011-11-03）. One of the most striking features of Phobos, aside from its irregular shape, is its giant crater Stickney. Because Phobos is only 28 by 20 km, the moon must have been nearly shattered from the force of the impact that caused the giant crater. Grooves that extend across the surface from Stickney appear to be surface fractures caused by the impact.
↑  Murray, J. B.;  et al.  (PDF). 37th Annual Lunar and Planetary Science Conference, March 2006.   [2011-11-07]. （原始内容存档 (PDF)于2011-11-22）.
↑  .   [2011-11-07]. （原始内容存档于2015-06-22）.
↑  Ivanov, Andrei V. . Solar System Research. March 2004, 38 (2): 97–107. Bibcode:2004SoSyR..38...97I. doi:10.1023/B:SOLS.0000022821.22821.84.
↑  Ivanov, Andrei; Michael Zolensky.  (PDF). Lunar and Planetary Science. 2003, 34  [2011-11-07]. （原始内容存档 (PDF)于2011-08-05）. The currently available data on the lithologic composition of the Kaidun meteorite– primarily the composition of the main portion of the meteorite, corresponding to CR2 carbonaceous chondrites and the presence of clasts of deeply differentiated rock – provide weighty support for considering the meteorite’s parent body to be a carbonaceous chondrite satellite of a large differentiated planet. The only possible candidates in the modern solar system are Phobos and Deimos, the moons of Mars.
↑  Sharma, B. K. . 2008-05-10. arXiv:0805.1454 .
↑  .   [2012-03-23]. （原始内容存档于2010-03-25）.
↑  Holsapple, K. A. . Icarus. December 2001, 154 (2): 432–448. Bibcode:2001Icar..154..432H. doi:10.1006/icar.2001.6683.
1 2 3  Burns, J. A. "Contradictory Clues as to the Origin of the Martian Moons," in Mars, H. H. Kieffer et al., eds., U. Arizona Press, Tucson, 1992
↑  .   [2011-11-07]. （原始内容存档于2012-01-14）. One idea is that Phobos and Deimos, Mars's other moon, are captured asteroids.
1 2  Landis, G. A. "Origin of Martian Moons from Binary Asteroid Dissociation," American Association for the Advancement of Science Annual Meeting; Boston, MA, 2001; 摘要 （页面存档备份，存于）.
↑  Cazenave, A.; Dobrovolskis, A.; Lago, B. . Icarus. 1980, 44 (3): 730–744. Bibcode:1980Icar...44..730C. doi:10.1016/0019-1035(80)90140-2.  引文使用过时参数coauthors (帮助)
↑  Martin Pätzold and Olivier Witasse. . ESA. 2010-03-04  [2010-03-04]. （原始内容存档于2010-03-07）.
↑  Craddock, R. A.; (1994); The Origin of Phobos and Deimos, 第25届月球和行星科学年会摘要（Abstracts of the 25th Annual Lunar and Planetary Science Conference，1994年3月14日至18日在休斯顿举办）293页
↑  Giuranna, M.; Roush, T. L.; Duxbury, T.; Hogan, R. C.; Geminale, A.; Formisano, V.  (PDF). . 2010  [2010-10-01]. （原始内容存档 (PDF)于2011-05-12）.  引文使用过时参数coauthors (帮助)
↑  . Space.com web site. 2010-09-27  [2010-10-01]. （原始内容存档于2010-09-30）.
1 2  Shklovsky, I. S.; The Universe, Life, and Mind, Academy of Sciences USSR, Moscow, 1962
↑  Öpik, E. J. . Irish Astronomical Journal. September 1964, 6: 281–283. Bibcode:1964IrAJ....6..281..
↑  Singer, S. F.; Astronautics, February 1960
1 2  Öpik, E. J. . Irish Astronomical Journal. March 1963, 6: 40. Bibcode:1963IrAJ....6R..40..
↑  Singer, S. F., , Seventh International Space Science Symposium held May 10–18, 1966 in Vienna, North-Holland Publishing Company, 1967, Bibcode:1967mopl.conf..317S
↑  "More on the Moons of Mars". Singer, S. F., Astronautics, February 1960. American Astronautical Society. Page 16
↑  "Cheap Flights to Phobos" by Stuart Clark, in New Scientist magazine, 2010年1月30日.
↑  . BBC News (London). 2010-03-04  [2010-03-07]. （原始内容存档于2010-03-07）.
↑  . NASA.   [2011-06-27]. （原始内容存档于2011-07-09）.
↑  . The Planetary Society.   [2010-03-12]. （原始内容存档于2010-02-17）.
↑  . RIA Novosti. 2006-09-11  [2010-03-12]. （原始内容存档于2013-08-17）.
↑  . Hong Kong Trader. 2007-05-01  [2010-05-12]. （原始内容存档于2012-02-13）.
↑  . Hong Kong Polytechnic University. 2007-04-02  [2010-05-12]. [永久]
↑  Amos, J.; Martian Moon ’Could be Key Test’ （页面存档备份，存于）, BBC News (2007年2月9日)
↑  Optech press release, "Canadian Mission Concept to Mysterious Mars moon Phobos to Feature Unique Rock-Dock Maneuver," 2007年5月3日.
↑  PRIME: Phobos Reconnaissance & International Mars Exploration 的存檔，存档日期2008-05-10., Mars Institute website, [2009年7月27日].
↑  Lee, P., R. Richards, A. Hildebrand, and the PRIME Mission Team 2008. The PRIME (Phobos Reconnaissance and International Mars Exploration) Mission and Mars sample Return. 39th Lunar Planet. Sci. Conf., Houston, TX, March 2008. [#2268]|http://www.lpi.usra.edu/meetings/lpsc2008/pdf/2268.pdf （页面存档备份，存于）
↑  原文：We should go boldly where man has not gone before. Fly by the comets, visit asteroids, visit the moon of Mars. There’s a monolith there. A very unusual structure on this potato shaped object that goes around Mars once in seven hours. When people find out about that they’re going to say ‘Who put that there? Who put that there?’ The universe put it there. If you choose, God put it there...
↑  . C-Span. 2009-07-22  [2012-03-23]. （原始内容存档于2012-03-13）.
↑  Mullen, Leslie. . Astrobiology Magazine (Space.com). 2009-04-30  [2009-09-05]. （原始内容存档于2009-08-05）.
↑  Lee, P. et al. 2010. Hall: A Phobos and Deimos Sample Return Mission. 44th Lunar Planet. Sci. Conf., The Woodlands, TX. 1-5 Mar 2010. [#1633] Bibcode：2010LPI....41.1633L.
↑  Landis, Geoffrey A. "Footsteps to Mars: an Incremental Approach to Mars Exploration," Journal of the British Interplanetary Society, Vol. 48, pp. 367-342 (1995); presented at Case for Mars V, Boulder CO, 26-May 29, 1993; appears in From Imagination to Reality: Mars Exploration Studies, R. Zubrin, ed., AAS Science and Technology Series Volume 91 pp. 339-350 (1997). （可以从Footsteps to Mars （页面存档备份，存于）访问，为PDF格式）
1 2  Lee, P., S. Braham, G. Mungas, M. Silver, P. Thomas, and M. West (2005). Phobos: A Critical Link Between Moon and Mars Exploration. Report of the Space Resources Rountable VII: LEAG Conference on Lunar Exploration, League City, TX 25-28 Oct 2005. LPI Contrib. 1318, p. 72. Bibcode：2005LPICo1287...56L
↑  Lee, P. (2007). Phobos-Deimos ASAP: A Case for the Human Exploration of the Moons of Mars. First Int’l Conf. Explor. Phobos & Deimos. NASA Research Park, Moffett Field, CA, 5-7 Nov 2007. LPI Contrib. 1377, p. 25 [#7044]|http://www.lpi.usra.edu/meetings/phobosdeimos2007/pdf/7044.pdf （页面存档备份，存于）
火卫一、火卫二的轨道示意图（成比例）。视角在火星北极上方。火卫一比火卫二的公转快3.96倍。
机遇号拍摄的火卫一凌日。
海盗1号拍摄的图像。斯蒂克尼陨石坑位于右侧。
在過去一段時間内，火衛一的影像品質已经有了很大的提高。这张圖片是對火星車和火星環繞飛行器拍攝的火衛一的影像的比较。
火卫一独石（中部偏右），由火星全球勘察者于1998年拍摄。（编号：MOC Image 55103）