Terrestrial-Type Xenon in Meteoritic Troilite
Abstract
Recently it has been realized that the isotopic composition of Xe in different phases of chondrites is not uniform and that AVCC Xe is a mixture of the different nucleogenetic components trapped in these phases1-4. We show here a similar abundance pattern for the nonradiogenic xenon isotopes in air and in meteoritic troilite (FeS), which suggests that the isotopic composition of atmospheric Xe was not produced by unique events in the history of terrestrial material but represents a particular mix of the different nucleogenetic components of Xe that was dominant in a central Fe- and S-rich region of the protoplanetary nebula5.
Recommended Citation
G. Hwaung and O. Manuel, "Terrestrial-Type Xenon in Meteoritic Troilite," Nature, vol. 299, pp. 807 - 810, Nature Publishing Group, Oct 1982.
The definitive version is available at https://doi.org/10.1038/299807a0
Department(s)
Chemistry
International Standard Serial Number (ISSN)
0028-0836
Document Type
Article - Journal
Document Version
Citation
File Type
text
Language(s)
English
Rights
© 1982 Nature Publishing Group, All rights reserved.
Publication Date
01 Oct 1982