Radionuclide studies of stony meteorites from hot deserts

A. J.Timothy Jull, Marlène D. Giscard, Aurore Hutzler, Caitlin J. Schnitzer, David Zahn, George S. Burr, Lanny R. McHargue, Dolores Hill

Research output: Contribution to journalArticle

1 Scopus citations

Abstract

We summarize the use of radiocarbon produced by spallation in meteorites in space to determine their terrestrial age or residence time. This "age" gives us important information as it can be compared to the rates of weathering and infall of meteorites. The processes that affect the collection of meteorites in a given area can be related to the rates of infall of new meteorites, and the rate of removal by chemical weathering and physical erosion.

Original languageEnglish (US)
Pages (from-to)1779-1789
Number of pages11
JournalRadiocarbon
Volume55
Issue number2-3
DOIs
StatePublished - Sep 25 2013

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Keywords

  • Cosmic rays
  • Meteorites
  • Terrestrial age

ASJC Scopus subject areas

  • Archaeology
  • Earth and Planetary Sciences(all)

Cite this

Jull, A. J. T., Giscard, M. D., Hutzler, A., Schnitzer, C. J., Zahn, D., Burr, G. S., McHargue, L. R., & Hill, D. (2013). Radionuclide studies of stony meteorites from hot deserts. Radiocarbon, 55(2-3), 1779-1789. https://doi.org/10.2458/azu_js_rc.55.16202