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Solar noble gases in the Angrite parent body – Evidence from volcanic volatiles trapped in D'Orbigny glass

Busemann, H.; Lorenzetti, S. and Eugster, O. (2004). Solar noble gases in the Angrite parent body – Evidence from volcanic volatiles trapped in D'Orbigny glass. In: 35th Lunar and Planetary Science Conference, 15-19 March 2004, Houston, Texas, USA.

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Abstract

We compare the noble gases in D'Orbigny glass and bulk. The glass was formed after the bulk silicates and contains interior solar noble gases that may originate from early volcanic activity on the angrite parent body, trapped upon fast cooling.

Item Type: Conference Item
Extra Information: Abstract #1705
Keywords: noble gases; angrites;
Academic Unit/Department: Science > Physical Sciences
Item ID: 8306
Depositing User: Kyra Proctor
Date Deposited: 02 Jul 2007
Last Modified: 20 Oct 2014 01:59
URI: http://oro.open.ac.uk/id/eprint/8306
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