Modal abundances of pyroxene, olivine, and mesostasis in nakhlites: Heterogeneity, variation, and implications for nakhlite emplacement

Author:

Corrigan Catherine M.1,Velbel Michael A.12,Vicenzi Edward P.3

Affiliation:

1. Department of Mineral Sciences; National Museum of Natural History; Smithsonian Institution; 10th St. and Constitution Ave. NW Washington District of Columbia 20013-7012 USA

2. Department of Geological Sciences; Michigan State University; East Lansing Michigan 48824 USA

3. Museum Conservation Institute; Smithsonian Institution; Suitland Maryland 20746 USA

Publisher

Wiley

Subject

Space and Planetary Science,Geophysics

Reference64 articles.

1. Experiments on a gravity-free dispersion of large solid spheres in a Newtonian fluid under shear;Bagnold;Royal Society of London Proceedings Series A,1954

2. Berkley J. L. Keil K. Prinz M. 1980 Comparative petrology and origin of Governador Valadares and other nakhlites 1089 1102

3. Martian meteorite chronology and the evolution of the interior of Mars;Bouvier;Earth and Planetary Science Letters,2009

4. The nakhlites, Part I: Petrography and mineral chemistry;Bunch;Meteoritics,1975

5. Corrigan C. M. Vicenzi E. P. Konicek A. R. Lunning N. 2011 An examination of the new Miller Range nakhlites (MIL 090030, 090032, and 090136) (abstract #2657)

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