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:||Science > Physical Sciences
|Depositing User:||Kyra Proctor|
|Date Deposited:||02 Jul 2007|
|Last Modified:||01 May 2016 08:03|
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