Busemann, H.; Lorenzetti, S. and Eugster, O.
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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:||Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
Faculty of Science, Technology, Engineering and Mathematics (STEM)
|Depositing User:||Kyra Proctor|
|Date Deposited:||02 Jul 2007|
|Last Modified:||25 Aug 2016 03:24|
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