In a recent Letter on a determination of the age of the elements, Reynolds[1] reported the important discovery of isotopically anomalous xenon in the stony meteorite Richarton. The isotopes which appear to occur in significant excess over atmospheric xenon are Xe128, Xe129, Xe130, and Xe131, with the Xe129 dominant by an order of magnitude. At present it does not appear possible to explain all of these data by any single mechanism. Because of the existence of these four anomalies, it is difficult to conclude that the Xe129 excess is simply the product of I129 decay
Nucleosynthetic anomalies have been observed in meteorites for many elements. The magnitude and repa...
Nucleosynthetic anomalies have been observed in meteorites for many elements. The magnitude and repa...
Analyses of noble gases in whole rock samples of the howardites Bholghati and Kapoeta and grain-size...
Specific nucleosynthetic environments are examined as the sources for the anomalous xenon observed i...
The general isotopic anomalies in meteoritic xenon are described in detail. Where superior isotopic ...
Analyses of noble gases from four natural gases reveal radiogenic He4 and Ar40, excess Ne21 and Ar38...
Analyses of noble gases from four natural gases reveal radiogenic He4 and Ar40, excess Ne21 and Ar38...
The abundance and isotopic composition of noble gases in meteorites is discussed in relation to the ...
The composition of Xe released from carbonaceous chondrites between 600 and 1000 C, particularly its...
Xenon isotope abundance data from other investigations have been analyzed with the aid of an IBM 704...
Nucleosynthetic anomalies have been observed in meteorites for many elements. The magnitude and repa...
The neon and xenon isotope anomalies observed in meteorites can be interpreted in terms of a mass fr...
Nucleosynthetic anomalies have been observed in meteorites for many elements. The magnitude and repa...
Nucleosynthetic anomalies have been observed in meteorites for many elements. The magnitude and repa...
Analyses of noble gases in whole rock samples of the howardites Bholghati and Kapoeta and grain-size...
Nucleosynthetic anomalies have been observed in meteorites for many elements. The magnitude and repa...
Nucleosynthetic anomalies have been observed in meteorites for many elements. The magnitude and repa...
Analyses of noble gases in whole rock samples of the howardites Bholghati and Kapoeta and grain-size...
Specific nucleosynthetic environments are examined as the sources for the anomalous xenon observed i...
The general isotopic anomalies in meteoritic xenon are described in detail. Where superior isotopic ...
Analyses of noble gases from four natural gases reveal radiogenic He4 and Ar40, excess Ne21 and Ar38...
Analyses of noble gases from four natural gases reveal radiogenic He4 and Ar40, excess Ne21 and Ar38...
The abundance and isotopic composition of noble gases in meteorites is discussed in relation to the ...
The composition of Xe released from carbonaceous chondrites between 600 and 1000 C, particularly its...
Xenon isotope abundance data from other investigations have been analyzed with the aid of an IBM 704...
Nucleosynthetic anomalies have been observed in meteorites for many elements. The magnitude and repa...
The neon and xenon isotope anomalies observed in meteorites can be interpreted in terms of a mass fr...
Nucleosynthetic anomalies have been observed in meteorites for many elements. The magnitude and repa...
Nucleosynthetic anomalies have been observed in meteorites for many elements. The magnitude and repa...
Analyses of noble gases in whole rock samples of the howardites Bholghati and Kapoeta and grain-size...
Nucleosynthetic anomalies have been observed in meteorites for many elements. The magnitude and repa...
Nucleosynthetic anomalies have been observed in meteorites for many elements. The magnitude and repa...
Analyses of noble gases in whole rock samples of the howardites Bholghati and Kapoeta and grain-size...