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Experimental Study into the Stability of Whitlockite and Hydroxylapatite in Basaltic MagmasApatite (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.
Document ID
20180002600
Acquisition Source
Johnson Space Center
Document Type
Conference Paper
Authors
McCubbin, F. M.
(NASA Johnson Space Center Houston, TX, United States)
Barnes, J. J.
(NASA Johnson Space Center Houston, TX, United States)
Vander Kaaden, K. E.
(Jacobs Technology, Inc. Houston, TX, United States)
Srinivasan, P.
(New Mexico Univ. Albuquerque, NM, United States)
Whitson, E. S.
(New Mexico Univ. Albuquerque, NM, United States)
Turner, A.
(Jacobs Technology, Inc. Houston, TX, United States)
Reppart, J. J.
(Jacobs Technology, Inc. Houston, TX, United States)
Date Acquired
April 27, 2018
Publication Date
March 19, 2018
Subject Category
Space Sciences (General)
Report/Patent Number
JSC-E-DAA-TN52118
Meeting Information
Meeting: Lunar and Planetary Science Conference
Location: Woodlands, TX
Country: United States
Start Date: March 19, 2018
End Date: March 23, 2018
Sponsors: Lunar and Planetary Inst.
Funding Number(s)
CONTRACT_GRANT: NNH15C048B
CONTRACT_GRANT: NNJ13HA01C
Distribution Limits
Public
Copyright
Public Use Permitted.
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