Experimental Study into the Stability of Whitlockite and Hydroxylapatite in Basaltic Magmas

McCubbin, F M ; Barnes, J J ; Vander Kaaden, K E ; Srinivasan, P ; Whitson, E S ; Turner, A ; Reppart, J J

关键词: CALCIUM PHOSPHATES;    METEORITES;    MINERALOGY;    MINERALS;    PHOSPHATES;    PLANETARY COMPOSITION;    ROCKS;    WATER;    ASTEROIDS;    CRYSTAL STRUCTURE;    LUNAR ROCKS;    MARS SURFACE SAMPLES;    MOON;    PHYSICAL CHEMISTRY;   

RP-ID  :  JSC-E-DAA-TN52118

学科分类：空间科学

美国|英语

来源: NASA Technical Reports Server

【 摘 要 】

Apatite (Ca5(PO4)3(F,Cl,OH)), merrillite (Ca18Na2Mg2(PO4)14), and whitlockite (Ca9(Mg,Fe(2+))(PO4)6[PO3(OH)]) are the primary phosphate minerals found in most planetary materials including rocks from Earth, Moon, Mars, and asteroids. For many years, the terms merrillite and whitlockite have been used interchangeably in the meteorite literature. Much of the confusion regarding the relationship between terrestrial and extraterrestrial 'whitlockite' is based on the presence or absence of hydrogen in the mineral structure. Whitlockite has approximately 8500 ppm H2O, and the term 'merrillite' has been adopted to identify the hydrogen-free form of whitlockite. The atomic structures of merrillite and whitlockite were examined in detail by Hughes et al.. On Earth, whitlockite has been found in rocks from evolved pegmatitic systems and in some mantle rocks. Furthermore, terrestrial whitlockite has been shown to have some merrillite component. For the meteoritic and lunar materials that have been investigated, merrillite appears to be far more common than whitlockite, and it has been proposed that the whitlockite component is unique to terrestrial samples. There are some reports of 'whitlockite' in the meteorite literature; however, these may represent misidentifications of merrillite because there have been no reports of extraterrestrial whitlockite that have been verified through crystal structural studies or analyzed for their H contents. Hughes et al. reported the atomic arrangement of lunar merrillite and demonstrated that the phase is similar to meteoritic merrillite and, predictably, devoid of hydrogen. In a follow-up study, Hughes et al. reported the atomic arrangements of two natural samples of whitlockite, one synthetic whitlockite, and samples of synthetic whitlockite that were heated at 500 C or 1050 C for 24 h. The crystal chemistry and crystal structures of the phases were compared, and it was discovered that the latter treatment resulted in the dehydrogenation of whitlockite to form merrillite.