Computer Science
Scientific paper
Jan 1991
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991gecoa..55...59s&link_type=abstract
(Workshop on Differences between Antarctic and non-Antarctic Meteorites, Vienna, Austria, July 27, 28, 1989) Geochimica et Cosmo
Computer Science
33
Antarctic Regions, Chondrites, Meteoritic Composition, Rare Gases, Argon Isotopes, Cosmic Rays, Helium Isotopes, Neon Isotopes, Meteorites, Antarctic Meteorites, Rare Gases, H Chondrites, Comparisons, Alh Meteorites, Laboratory Studies, Exposure Age, Pairing, Helium 4, Argon 40, Catalog, Concentration, Abundance, Nuclides, Neon 21, Gases, Radiogenic Material, Distribution, Petrography, Terrestrial Age, Isotopes
Scientific paper
Thirty-one Antarctic H-chondrites from the Allan Hills have been analyzed for their noble gases. Seven of the specimens contain solar gases; 13 have a cosmic-ray exposure age around 8 Ma. Both fractions are as observed for H-chondrites from the rest of the world. Scrutiny of the data for 'paired samples' yields a minimum number of 17 independent falls, with six falls required for the 8 Ma peak of exposure age. The distribution of exposure ages as well as that of radiogenic He-4 and Ar-40 yield no evidence that H-chondrites from the Allan Hills region represent a mixture of populations that is different from that brought to moderate latitudes of the earth in more recent times.
Begemann Friedrich
Schultz Ludolf
Weber Harald W.
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