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Genesis of Augite-Bearing Ureilites: Evidence From LA-ICP-MS Analyses of Pyroxenes and OlivineUreilites are ultramafic achondrites composed primarily of coarse-grained low-Ca pyroxene and olivine with interstitial carbonaceous material, but a number of them contain augite [1]. Ureilites are considered to be restites after partial melting of a chondritic precursor, although at least some augite-bearing ureilites may be partially cumulate [1, 2]. In this scenario, the augite is a cumulus phase derived from a melt that infiltrated a restite composed of typical ureilite material (olivine+low-Ca pyroxene) [2]. To test this hypothesis, we examined the major and trace element compositions of silicate minerals in select augite-bearing ureilites with differing mg#. Polished thick sections of the augite-bearing ureilites ALH 84136 , EET 87511, EET 96293, LEW 88201, and META78008 and augite-free typical ureilite EET 90019 were examined by EPMA for major and minor elements and laser ablation ICP-MS (LA-ICP-MS) for trace elements, REE in particular. Although EET 87511 is reported to contain augite, the polished section that we obtained did not.
Document ID
20080010778
Acquisition Source
Johnson Space Center
Document Type
Extended Abstract
Authors
Herrin, J. S.
(NASA Johnson Space Center Houston, TX, United States)
Lee, C-T. A.
(Rice Univ. Houston, TX, United States)
Mittlefehldt, D. W.
(NASA Johnson Space Center Houston, TX, United States)
Date Acquired
August 24, 2013
Publication Date
January 1, 2008
Subject Category
Geophysics
Meeting Information
Meeting: 39th Lunar and Planetary Science Conference
Location: League City, TX
Country: United States
Start Date: March 10, 2008
End Date: March 14, 2008
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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