Petrography, composition, and origin of large, chromian spinels from the Murchison meteorite
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Dual Isotopic Composition of Methane in Murchison Meteorite
Introduction: Examining the record contained within the organic matter in meteorites can reveal the nature of the inputs and processes that contributed to the early solar system environment. Specifically, isotopic measurements for individual organic compounds can reveal the reaction mechanisms and possible source environments from which the organic constituents were formed. Hydrogen isotopic me...
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Murchisite (IMA 2010-003), Cr5S6, is a new chromium sulfide mineral, discovered in the Murchison CM2 meteorite. The type material occurs as one subhedral crystal (1.3 × 4 mm in size) in contact with low-Ni iron (“kamacite”), martensitic iron, schreibersite, and a Ca-,Al-rich glass, all of which are included in an isolated forsteritic olivine grain in the meteorite’s matrix. The mean chemical co...
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MURCHISON METEORITE. F. Gyngard 1 , J. N. Ávila 2,3 , T. R. Ireland 2,3 , and E. Zinner 1 , 1 Laboratory for Space Sciences and Department of Physics, [email protected], Washington University, St. Louis, MO 63130, USA, 2 Research School of Earth Sciences, The Australian National University, Canberra ACT 0200, Australia, 3 Planetary Science Institute, The Australian National University, Canberr...
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Article history: Carbon-rich meteorites, car Received 26 October 2007 Received in revised form 7 March 2008 Accepted 11 March 2008 Available online 20 March 2008 Editor: R.D. van der Hilst
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ژورنال
عنوان ژورنال: Geochimica et Cosmochimica Acta
سال: 1994
ISSN: 0016-7037
DOI: 10.1016/0016-7037(94)90384-0