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Oxygen Isotopic Constraints on the Number and Origin of Basaltic Achondrite Parent Bodies

Scott, E. R. D.; Greenwood, R. C.; Franchi, I. A.; Barrat, J. A. and Sanders, I. S. (2008). Oxygen Isotopic Constraints on the Number and Origin of Basaltic Achondrite Parent Bodies. In: 39th Lunar and Planetary Science Conference (Lunar and Planetary Science XXXIX), 10-14 Mar 2008, League City, Texas, USA, Lunar and Planetary Institute, p. 2344.

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Abstract

Our data show that HED meteorites have a homogeneous oxygen isotopic composition consistent with a magma ocean on Vesta. Ibitira, Asuka 881394, Pasamonte, and NWA 1240 probably come from separate parent asteroids.

Item Type: Conference or Workshop Item
Extra Information: Abstract #2344
Academic Unit/School: Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
Faculty of Science, Technology, Engineering and Mathematics (STEM)
Item ID: 12490
Depositing User: Ian Franchi
Date Deposited: 02 Dec 2008 06:17
Last Modified: 13 Dec 2018 03:03
URI: http://oro.open.ac.uk/id/eprint/12490
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