Both lunar and terrestrial rocks are made up of minerals. Lunar minerals’ atomic structures and compositions provided the keys to understanding the lunar rock-forming chemical and physical environments. Analyses of lunar minerals have enabled scientists to determine some key parameters, like temperature, pressure, cooling rate, and partial pressures of gases existed during the formation of rocks.
Generally, lunar minerals can be classified into six main groups (Fig. 1).
References
Anderson AT Jr, Bunch TE, Cameron EN, Haggerty SE, Boyd FR, Finger LW, James OB, Keil K, Prinz M, Ramdohr P, El Goresy A (1970) Armalcolite: a new mineral from the Apollo 11 samples. In: Proceedings of the Apollo 11 lunar science conference, pp 55–63
BVSP (Basaltic Volcanism Study Project) (1981) Basaltic volcanism on the terrestrial planets. Pergamon, New York, 1286 pp
Champness PE, Dunham AC, Gibb FGF, Giles HN, MacKenzie WS, Stumpfl EF, Zussman J (1971) Mineralogy and petrology of some Apollo 12 samples. In: Proceedings of the second lunar science conference, pp 359–376
Dence MR, Douglas JAV, Plant AG, Traill RJ (1970) Petrology, mineralogy and deformation of Apollo 11 samples. In: Proceedings of the Apollo 11 lunar science conference, pp 315–340
El Goresy A, Ramdohr P, Taylor LA (1971) The geochemistry of the opaque minerals in Apollo 14 crystalline rocks. Earth Planet Sci Lett 13:121–129
Greenwood JP, Itoh S, Sakamoto N, Warren P, Taylor L, Yurimoto H (2011) Hydrogen isotope ratios in lunar rocks indicate delivery of cometary water to the Moon. Nature Geoscience 4:79–82
Papike JJ, Cameron M (1976) Crystal chemistry of silicate minerals of geophysical interest. Rev Geophys Space Phys 14:37–80
Papike JJ, Hodges FN, Bence AE, Cameron M, Rhodes JM (1976) Mare basalts: crystal chemistry, mineralogy, and petrology. Rev Geophys Space Phys 14:475–540
Ramdohr P, El Goresy A (1970) Opaque minerals of the lunar rocks and dust from Mare Tranquillitatis. Science 167:615–618
Reid AM, Meyer C, Harmon RS, Brett R (1970) Metal grains in Apollo 12 igneous rocks. Earth Planet Sci Lett 9:1–5
Sha LK (2000) Whitlockite solubility in silicate melts: some insights into lunar and planetary evolution. Geochim Cosmochim Acta 64:3217–3236. doi:10.1016/S0016-7037(00)00420-8
Sippel RF (1971) Luminescence petrography of the Apollo 12 rocks and comparative features in terrestrial rocks and meteorites. In: Proceedings of the second lunar science conference, pp 247–263
Skinner BJ (1970) High crystallization temperatures indicated for igneous rocks from tranquillity base. Proceedings of the Apollo 11 lunar science conference, pp 891–895
Taylor LA (1988) Generation of native Fe in lunar soil. In: Johnson SW, Wetzel JP (eds) Engineering, construction, and operations in space: proceedings of space ‘88. American Society of Civil Engineers, New York, pp 67–77
Taylor LA, Kullerud G, Bryan WB (1971) Opaque mineralogy and textural features of Apollo 12 samples and a comparison with Apollo 11 rocks. In: Proceedings of the second lunar science conference, pp 855–871
Vaniman DT, Papike JJ (1980) Lunar highland melt rocks: chemistry petrology and silicate mineralogy. In: Papike JJ, Merrill RB (eds) Proceedings of the conference on the lunar highlands crust. Pergamon, New York, pp 271–337
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Huang, Z. (2017). Lunar Mineral Distribution. In: Cudnik, B. (eds) Encyclopedia of Lunar Science. Springer, Cham. https://doi.org/10.1007/978-3-319-05546-6_55-1
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