Petrography and Origin of the Unique Achondrite GRA 06128 and 06129: Preliminary ResultsGRA 06128 & 06129 are paired achondrites [1], with unique mineral proportions (75% oligoclase), mineral compositions, and oxygen isotope ratios. They appear to represent alkalic igneous rock from a hitherto unsampled differentiated parent body, modified significantly by thermal and shock metamorphism. Samples and Methods: Bulk samples were examined at JSC during splitting for consortium analyses. Microscope and BSE images here are on thick section GRA06128,40. Chemical analyses of minerals were acquired at Johnson Space Center with the Cameca SX100, operated at 15 kV. Feldspar was analyzed with a defocused 5 micron beam @ 5 nA; other minerals were analyzed with a focused beam @ 20 nA. Moessbauer spectra were obtained at ARES, JSC [2]. Intrinsic radioactivity was measured in the low-level counting facility at ARES JSC [3]. An estimated abundance of Al-26 of approx. 70 dpm/kg is within the range determined for eucrites.
Document ID
20080009712
Acquisition Source
Johnson Space Center
Document Type
Extended Abstract
Authors
Treiman, A. H. (Lunar and Planetary Inst. Houston, TX, United States)
Morris, R. V. (NASA Johnson Space Center Houston, TX, United States)
Kring, D. A. (Lunar and Planetary Inst. Houston, TX, United States)
Mittlefehldt, D. W. (NASA Johnson Space Center Houston, TX, United States)
Jones, J. H. (NASA Johnson Space Center Houston, TX, United States)
Date Acquired
August 24, 2013
Publication Date
January 1, 2008
Subject Category
Geophysics
Meeting Information
Meeting: 39th Lunar and Planetary Science Conference