Eugster, O.; Busemann, H.; Kurat, G.; Lorenzetti, S. and Varela, M. E.
PDF (Not Set)
- Requires a PDF viewer such as GSview, Xpdf or Adobe Acrobat Reader
|Google Scholar:||Look up in Google Scholar|
Introduction: The D’Orbigny angrite, a 16.55 kg stone, was found 1979 in Argentina . Mineralogy and chemistry of this meteorite were characterized in detail [2-6]. A Pb-U-Th age of 4.559 Ga was obtained for pyroxenes by Jagoutz et al. . Here we report results on the noble gas isotopic composition and, in particular, on the cosmic-ray exposure (CRE) age of D’Orbigny.
|Item Type:||Conference Item|
|Extra Information:||Abstract #5077|
|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:||26 Oct 2016 12:10|
|Share this page:|
Download history for this item
These details should be considered as only a guide to the number of downloads performed manually. Algorithmic methods have been applied in an attempt to remove automated downloads from the displayed statistics but no guarantee can be made as to the accuracy of the figures.