April, 2000 |
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Los Angeles 001A New Martian Shergottite![]() Analysis and description by:Russell Kempton, New England Meteoritical ServicesLos Angeles 001, paired with Los Angeles 002, represents the 14th verified Martian meteorite. This new addition to our collection of rocks from Mars has been classified as a basaltic shergottite (the fifth one after Shergotty, Zagami, EETA79001, and QUE94201) and is the most geochemically evolved sample of the Martian surface found to date on Earth. Los Angeles 001 is unusually coarse-grained indicating that it cooled from igneous temperatures (1200 C to 900 C) at a slower rate than other shergottites. This slower cooling resulted in a crystallization of the pyroxenes augite and pigeonite in lamellae easily visible to the unaided eye. In comparison, the augite in Zagami is almost an order of magnitude smaller than that observed in LA001. ![]() Augite and pigeonite lamellae![]() Augite within pigeoniteLos Angeles 001 fusion crust and exterior![]() ![]() Fusion crust visible on the outside surface![]() For a better understanding of Fusion Crust |
This slice of LA001 was sent to us by a NEMS customer who had purchased it elsewhere. The customer asked us to remove the "saw blade" cutting marks from the specimen and allowed us to extensively photograph it. References: Warren P.H. et al. "Geochemistry of Los Angeles, a Ferroan, La- and Th-Rich Basalt From Mars", 2000, LPSC31 Rubin A.E. et al. "Petrology of Los Angeles: A New Basaltic Shergottite Find", 2000, LPSC31 Photographs Copyright © 2000, New England Meteoritical Services. Index |