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Discovery of Abundant Tremolite in a Carbonaceous Chondrite Fragment from the Almahata Sitta MeteoriteAlmahata Sitta (AhS) is classified as an anomalous, polymict ureilite and was observed prior to Earth impact as the F-type asteroid 2008 TC3 [e.g., 1-2]. As part of our characterization of this unusual meteorite [e.g., 3], we have been using microscopic infrared spectroscopy (µ-FTIR) to measure the mineralogy of fragments identified as carbonaceous chondrites (CC). In fragment 202 we have discovered unambiguous spectral evidence for a minimum of several vol% amphibole (specifically, tremolite), a mineral that is not known to occur in volumetrically significant abundances (defined here as >1%) in carbonaceous chondrites
Document ID
20200001829
Acquisition Source
Johnson Space Center
Document Type
Abstract
Authors
Hamilton, V. E.
(Southwest Research Inst. Boulder, CO, United States)
Goodrich, C. A.
(Lunar and Planetary Institute (LPI) Houston, TX, United States)
Treiman, A.
(Lunar and Planetary Institute (LPI) Houston, TX, United States)
Connolly, H. C., Jr.
(Rowan Univ. Glassboro, NJ, United States)
Zolensky, M. E.
(NASA Johnson Space Center Houston, TX, United States)
Shaddad, M.
(Khartoum Univ. Sudan)
Date Acquired
March 19, 2020
Publication Date
March 16, 2020
Subject Category
Space Sciences (General)
Report/Patent Number
JSC-E-DAA-TN77013
Report Number: JSC-E-DAA-TN77013
Meeting Information
Meeting: Lunar and Planetary Science Conference
Location: The Woodlands, TX
Country: United States
Start Date: March 16, 2020
End Date: March 20, 2020
Sponsors: Lunar and Planetary Institute (LPI)
Distribution Limits
Public
Copyright
Public Use Permitted.
Technical Review
Single Expert
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