Descartesites - Missing(?) pristine rocks

Details Descartesites - Missing(?) pristine rocks Descartesites - Missing(?) pristine rocks

Mar 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997lpi....28..829l&link_type=abstract

Conference Paper, 28th Annual Lunar and Planetary Science Conference, p. 829.

Computer Science

Pyroxenes, Lunar Composition, Anorthosite, Magma, Silicon Dioxide, Crystallization, Iron Oxides, Magnesium Oxides

Scientific paper

A thermal divide that is stable to comparatively low temperatures in lunar compositions because of their low alkalies is presently invoked in order to explain the absence of granitoids called 'descartesites' which are residual to the formation of lunar ferroan anorthosites (FANs). Attention is given to the composition paths generated by fractional crystallization of a model FAN parent liquid at pressures of 0 and 3 kb.

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