@article{oai:nipr.repo.nii.ac.jp:00004544,
 author = {Takaoka,Nobuo and Yoshida,Yo-ichi},
 journal = {Proceedings of the NIPR Symposium on Antarctic Meteorites},
 month = {Mar},
 note = {P(論文), Unique meteorite Yamato-74063 contains large amounts of trapped heavy noble gases whereas it is depleted in trapped He and Ne. The concentration of trapped ^<36>Ar is comparable with that of E- and C-chondrites and ureilites. Trapped ^<132>Xe is unusually abundant. Y-74063 contains a very high concentration of radiogenic ^<129>Xe. Trapped ^<20>Ne/^<36>Ar is low and similar to that of ureilites. Trapped ^<36>Ar/^<132>Xe of 32±4 is lower than that of any meteorites ever reported. The trapped gases in Y-74063 are depleted in Ar relative to Xe. Planetary-type noble gases may be mixtures of an Ar-depleted component and the "sub-solar" or "Ar-rich" component isolated in E-chondrites. The cosmic-ray exposure age is 6.2±0.4 Ma. Gas-retention ages are calculated to be less than 3.7±0.2,and 4.8±0.4 Ga from radiogenic ^4He and ^<40>Ar respectively. The K-Ar age older than the age of the solar system may attributed to chemical inhomogeneities resulting in an exceptionally high K concentration of the investigated sample. The gasretention ages, the large amounts of radiogenic ^<129>Xe and the trapped noble gases indicate that the meteorite was a closed system for the noble gases since crystallization.},
 pages = {178--186},
 title = {Noble gas composition in unique meteorite Yamato-74063},
 volume = {4},
 year = {1991}
}