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Cooling History of Almahata Sitta Ureilite as Inferred from Transmission Electron Microscopy of Iron MetalAlmahata Sitta (AS) is a polymict breccia mainly composed of various ureilite lithologies with lesser chondritic lithologies [1]. In the ureilite lithologies, Fe metal is a common accessory phase present either as large grain boundary grains or small particles formed by reduction of olivine and pyroxene. In our earlier studies on grain boundary metals in one of AS fragments (#44) we found unique features never seen in other ureilites [2,3]. In order to further characterize these metal grains, we performed a detailed TEM study on a FIB section prepared from one of AS #44 grain boundary metals and here discuss its thermal history.
Document ID
20140000761
Acquisition Source
Johnson Space Center
Document Type
Conference Paper
Authors
Mikouchi, T.
(Tokyo Univ. Japan)
Aoyagi, Y.
(Tokyo Univ. Japan)
Goodrich, C. A.
(Planetary Science Inst. Tucson, AZ, United States)
Yubuta, K.
(Tohoku Univ. Sendai, Japan)
Sugiyama, K.
(Tohoku Univ. Sendai, Japan)
Zolensky, M. E.
(NASA Johnson Space Center Houston, TX, United States)
Goldstein, J. I.
(Massachusetts Univ. Amherst, MA, United States)
Date Acquired
February 18, 2014
Publication Date
July 29, 2013
Subject Category
Geophysics
Report/Patent Number
Report Number: JSC-CN-28793
Report Number: JSC-CN-28793
JSC-CN-28793
JSC-CN-28793
Meeting Information
Meeting: 2013 Meteoritical Society Meeting
Location: Edmonton
Country: Canada
Start Date: July 29, 2013
End Date: August 2, 2013
Sponsors: Meteoritical Society
Distribution Limits
Public
Copyright
Public Use Permitted.
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