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)