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Mineralogical Study of a White Clast from Murchison (CM2): Comparison with R-ChondritesR-chondrites share some properties with ordinary chondrites (OC) and carbonaceous chondrites (CC). The proportions of the textural types of chondrule from R chondrites and their FeO/(FeO+MgO) ratios are similar to those of OC, but the high matrix abundance in R chondrites more closely resembles that of CC (matrix abundances: OC ~12 vol% vs. CC 34->60 vol%;). In this study, we characteristize the mineralogy of a white clast from Murchison (CM2), which was earlier considered to be a R-chondrite. First, all the petrographic and mineralogical characteristics will be described and compared with those of R-chondrites. Finally, all data will be considered in order to test, whether this clast is a real R-chondrite or a unique recrystallized chondrite?
Document ID
20180006498
Acquisition Source
Johnson Space Center
Document Type
Conference Paper
Authors
Kerraouch, I.
(Universite des Sciences et de la Technologie Houari Boumediene Algiers, Algeria)
Zolensky, M. E.
(NASA Johnson Space Center Houston, TX, United States)
Bischoff, A.
(Muenster Univ. Germany)
Le, L.
(Jacobs Technologies Engineering Science Contract Group Houston, TX, United States)
Belhai, D.
(Universite des Sciences et de la Technologie Houari Boumediene Algiers, Algeria)
Patzek, M.
(Muenster Univ. Germany)
Ebert, S.
(Muenster Univ. Germany)
Date Acquired
October 18, 2018
Publication Date
July 22, 2018
Subject Category
Space Sciences (General)
Report/Patent Number
JSC-E-DAA-TN56759
Meeting Information
Meeting: Annual Meeting of The Meteoritical Society
Location: Moscow
Country: Russia
Start Date: July 22, 2018
End Date: July 27, 2018
Sponsors: Meteoritical Society
Distribution Limits
Public
Copyright
Public Use Permitted.
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