The I-Xe chronometer and its constraints on the accretion and evolution of planetesimals
Author:
Affiliation:
1. School of Earth and Environmental Science, University of Manchester
Publisher
Geochemical Society of Japan
Subject
Geochemistry and Petrology,Geophysics
Link
https://www.jstage.jst.go.jp/article/geochemj/51/1/51_2.0429/_pdf
Reference52 articles.
1. Amelin, Y. (2001) U-Pb chronology of chondritic pyroxenes (abstract #1389). 32nd Lunar and Planetary Science Conference.
2. Amelin, Y., Ghosh, A. and Rotenberg, E. (2005) Unraveling the evolution of chondrite parent asteroids by precise U-Pb dating and thermal modelling. Geochim. Cosmochim. Acta 69, 505–518.
3. Anders, E. and Grevesse, N. (1989) Abundances of the elements—meteoritic and solar. Geochim. Cosmochim. Acta 53, 197–214.
4. Bernatowicz, T. J., Podosek, F. A., Swindle, T. D. and Honda, M. (1988) I-Xe systematics in LL chondrites. Geochim. Cosmochim. Acta 52, 1113–1121.
5. Bland, P. A., Collins, G. S., Davison, T. M., Abreu, N. M., Ciesla, F. J., Muxworthy, A. R. and Moore, J. (2014) Pressure-temperature evolution of primordial solar system solids during impact-induced compaction. Nature Communications 5, 1–13.
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