Element distribution and noble gas isotopic abundances in lunar meteorite Allan Hills A81005

• Main Authors: Kraehenbuehl, U., Eugster, O., Niedermann, S.
• Format: Other/Unknown Material
• Language: unknown
• Published: 1986
• Subjects: ASTROPHYSICS; Antarctic; Allan Hills; Antarc*
• Online Access: http://hdl.handle.net/2060/19860019349

Antarctic meteorite ALLAN HILLS A81005, an anorthositic breccia, is recognized to be of lunar origin. The noble gases in this meteorite were analyzed and found to be solar-wind implanted gases, whose absolute and relative concentrations are quite similar to those in lunar regolith samples. A sample of this meteorite was obtained for the analysis of the noble gas isotopes, including Kr(81), and for the determination of the elemental abundances. In order to better determine the volume derived from the surface correlated gases, grain size fractions were prepared. The results of the instrumental measurements of the gamma radiation are listed. From the amounts of cosmic ray produced noble gases and respective production rates, the lunar surface residence times were calculated. It was concluded that the lunar surface time is about half a billion years.