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 Mar 2004, Houston, Texas, USA.

URL: http://www.lpi.usra.edu/meetings/lpsc2004/pdf/1705...

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.

Viewing alternatives

Item Actions

Export

You can export this page using these formats