فوبوس
مراجع

1 2 3 4 5 6 7  "Mars: Moons: Phobos". NASA Solar System Exploration. 30 سبتمبر 2003. مؤرشف من الأصل في 2015-09-18. اطلع عليه بتاريخ 2013-12-02.
↑  "Planetary Satellite Physical Parameters". مختبر الدفع النفاث (Solar System Dynamics). 13 يوليو 2006. مؤرشف من الأصل في 2019-01-04. اطلع عليه بتاريخ 2008-01-29.
↑  Campbell، W.W. (1918). "The Beginning of the Astronomical Day". Publications of the Astronomical Society of the Pacific. ج. 30 ع. 178: 358. Bibcode:1918PASP...30..358C. DOI:10.1086/122784.
↑  "Notes: The Satellites of Mars". The Observatory. ج. 1 ع. 6: 181–185. 20 سبتمبر 1877. Bibcode:1877Obs.....1..181. مؤرشف من الأصل في 2020-10-01. اطلع عليه بتاريخ 2009-02-04.
↑  Hall، Asaph (17 أكتوبر 1877). "Observations of the Satellites of Mars". Astronomische Nachrichten (Signed 21 September 1877). ج. 91 ع. 2161: 11/12–13/14. Bibcode:1877AN.....91...11H. DOI:10.1002/asna.18780910103. مؤرشف من الأصل في 2020-05-11.
↑  Morley، Trevor A. (فبراير 1989). "A Catalogue of Ground-Based Astrometric Observations of the Martian Satellites, 1877–1982". Astronomy and Astrophysics Supplement Series. ج. 77 ع. 2: 209–226. Bibcode:1989A&AS...77..209M. مؤرشف من الأصل في 2020-07-29. (Table II, p. 220: first observation of Phobos on 18 August 1877.38498)
↑  Madan، Henry George (4 أكتوبر 1877). "Letters to the Editor: The Satellites of Mars". Nature (Signed 29 September 1877). ج. 16 ع. 414: 475. Bibcode:1877Natur..16R.475M. DOI:10.1038/016475b0. مؤرشف من الأصل في 2020-08-01.
↑  Hall، Asaph (14 مارس 1878). "Names of the Satellites of Mars". Astronomische Nachrichten (Signed 7 February 1878). ج. 92 ع. 2187: 47–48. Bibcode:1878AN.....92...47H. DOI:10.1002/asna.18780920304. مؤرشف من الأصل في 2020-07-29.
↑  Fanale، Fraser P.؛ Salvail، James R. (1989). "Loss of water from Phobos". Geophys. Res. Lett. ج. 16 ع. 4: 287–290. Bibcode:1989GeoRL..16..287F. DOI:10.1029/GL016i004p00287.
↑  Fanale، Fraser P.؛ Salvail، James R. (ديسمبر 1990). "Evolution of the water regime of Phobos". Icarus. ج. 88 ع. 2: 380–395. Bibcode:1990Icar...88..380F. DOI:10.1016/0019-1035(90)90089-R.
↑  "Porosity of Small Bodies and a Reassesment [كذا] of Ida's Density". مؤرشف من الأصل في 2007-09-26. When the error bars are taken into account, only one of these, Phobos, has a porosity below 0.2...
↑  "Close Inspection for Phobos". مؤرشف من الأصل في 2013-03-10. It is light, with a density less than twice that of water, and orbits just 5,989 كيلومتر (3,721 mi) above the Martian surface.
↑  Busch، Michael W.؛ Ostro، Steven J.؛ Benner، Lance A. M.؛ Giorgini، Jon D.؛ وآخرون (2007). "Arecibo Radar Observations of Phobos and Deimos". Icarus. ج. 186 ع. 2: 581–584. Bibcode:2007Icar..186..581B. DOI:10.1016/j.icarus.2006.11.003.
↑  "Phobos". مؤرشف من الأصل في 2009-04-22.
↑  "Stickney Crater-Phobos". مؤرشف من الأصل في 2020-10-31. 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 كيلومتر (17 by 12 mi), it 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.
↑  Gough، Evan (20 نوفمبر 2018). "Strange Grooves on Phobos Were Caused by Boulders Rolling Around on its Surface". Universe Today. مؤرشف من الأصل في 2020-11-08. اطلع عليه بتاريخ 2018-11-21.
↑  Murray، John B.؛ Murray، John B.؛ Iliffe، Jonathan C.؛ Muller، Jan-Peter A. L.؛ وآخرون. "New Evidence on the Origin of Phobos' Parallel Grooves from HRSC Mars Express" (PDF). 37th Annual Lunar and Planetary Science Conference, March 2006. مؤرشف من الأصل (PDF) في 2020-10-25.
↑  Ivanov، Andrei؛ Zolensky، Michael (2003). "The Kaidun Meteorite: Where Did It Come From?" (PDF). Lunar and Planetary Science. ج. 34. مؤرشف من الأصل (PDF) في 2020-09-21. 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.
↑  Ivanov، Andrei V. (مارس 2004). "Is the Kaidun Meteorite a Sample from Phobos?". Solar System Research. ج. 38 ع. 2: 97–107. Bibcode:2004SoSyR..38...97I. DOI:10.1023/B:SOLS.0000022821.22821.84.
↑  Nola Taylor Redd (8 ديسمبر 2017). "Phobos: Facts About the Doomed Martian Moon". مؤرشف من الأصل في 2018-03-19.