The concentrations of rare gases and isotopic compositions of He, Ne and Ar were determined for fourteen chondrites and two achondrites from Antarctica. The Xe isotopic ratios were also determined for seven meteorites. Cosmic-ray exposure and gas retention ages are given. Exposure age of 55Ma determined for Y-75015 eucrite is longer than those for most eucrites so far reported. Xe contained in chondrites is a mixture of cosmogenic and trapped components. ^(Xe) excess from extinct ^I was found for these chondrites. In Y-75015 eucrite, trapped and cosmogenic Xe\u27s were dominant and an appreciable amount of fissiogenic Xe was detected. Five groups of paired meteorites are suggested on the basis of rare gas data
The isotopic compositions have been measured mass spectrometrically for neon, argon, krypton and xen...
Petrographical studies indicate that most meteorites collected from the Antarctic ice sheets are L a...
We performed a comprehensive study of the noble gas isotopic abundances in thirty-six chondrites inc...
Concentrations and isotopic ratios of five stable rare gases were determined in six antarctic meteor...
The concentrations of rare gases and isotopic compositions of He, Ne and Ar were determined in twent...
Here we present the abundances and isotopic compositions of the noble gases He, Ne, Ar, Kr, and Xe i...
Yamato-7301 (H4 chondrite) and Yamato-7304 and -7305 (both L5 chondrites) were investigated for conc...
Concentrations of noble gases and isotopic compositions of He, Ne and Ar were determined for small Y...
Yamato-74063 : The correlation in a three-isotope plot of Ne indicates Ne-A as the trapped component...
We measured the concentrations and isotopic compositions of He, Ne, and Ar in 14 fragments from 12 d...
Belgica-7904 (C2) carbonaceous chondrite was analyzed for rare gas isotopic compositions with stepwi...
We present concentration and isotopic composition of He, Ne, and Ar in ten chondrites from the Nulla...
We measured the concentrations and isotopic compositions of He, Ne, Ar, Kr, and Xe in a 60.36 mg sam...
The noble gases He, Ne, Ar, and Xe were measured in 27 individual Antarctic micrometeorites (AMMs) i...
The 13th Symposium on Polar Science/Ordinary sessions [OA] Antarctic meteorites, Thu. 17 Nov
The isotopic compositions have been measured mass spectrometrically for neon, argon, krypton and xen...
Petrographical studies indicate that most meteorites collected from the Antarctic ice sheets are L a...
We performed a comprehensive study of the noble gas isotopic abundances in thirty-six chondrites inc...
Concentrations and isotopic ratios of five stable rare gases were determined in six antarctic meteor...
The concentrations of rare gases and isotopic compositions of He, Ne and Ar were determined in twent...
Here we present the abundances and isotopic compositions of the noble gases He, Ne, Ar, Kr, and Xe i...
Yamato-7301 (H4 chondrite) and Yamato-7304 and -7305 (both L5 chondrites) were investigated for conc...
Concentrations of noble gases and isotopic compositions of He, Ne and Ar were determined for small Y...
Yamato-74063 : The correlation in a three-isotope plot of Ne indicates Ne-A as the trapped component...
We measured the concentrations and isotopic compositions of He, Ne, and Ar in 14 fragments from 12 d...
Belgica-7904 (C2) carbonaceous chondrite was analyzed for rare gas isotopic compositions with stepwi...
We present concentration and isotopic composition of He, Ne, and Ar in ten chondrites from the Nulla...
We measured the concentrations and isotopic compositions of He, Ne, Ar, Kr, and Xe in a 60.36 mg sam...
The noble gases He, Ne, Ar, and Xe were measured in 27 individual Antarctic micrometeorites (AMMs) i...
The 13th Symposium on Polar Science/Ordinary sessions [OA] Antarctic meteorites, Thu. 17 Nov
The isotopic compositions have been measured mass spectrometrically for neon, argon, krypton and xen...
Petrographical studies indicate that most meteorites collected from the Antarctic ice sheets are L a...
We performed a comprehensive study of the noble gas isotopic abundances in thirty-six chondrites inc...