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Presolar diamonds in Krymka: C, N and Xe isotope data from grain-size separates and comparison with other meteorites

Verchovsky, A. B; Fisenko, A. V.; Semjonova, L. F.; Wright, I. P. and Pillinger, C. T. (2004). Presolar diamonds in Krymka: C, N and Xe isotope data from grain-size separates and comparison with other meteorites. In: 35th Lunar and Planetary Science Conference, 15-19 March 2004, Houston, Texas, USA.

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Abstract

Comparison of carbon isotope variations in grain size fractions of presolar diamonds separated from three meteorites (Efremovka, Boriskino and Krymka) suggest that diamond from various parts of solar nebular have had diffrent C isotope signature.

Item Type: Conference Item
Extra Information: Abstract #1673
Academic Unit/Department: Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
Faculty of Science, Technology, Engineering and Mathematics (STEM)
Interdisciplinary Research Centre: Centre for Earth, Planetary, Space and Astronomical Research (CEPSAR)
Item ID: 8763
Depositing User: Kyra Proctor
Date Deposited: 20 Jul 2007
Last Modified: 04 Aug 2016 06:22
URI: http://oro.open.ac.uk/id/eprint/8763
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