40Ar-39Ar ages of H-chondrite impact melt breccias

Timothy Swindle, Clark E. Isachsen, John R. Weirich, David A. Kring

Research output: Contribution to journalArticle

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Abstract

40Ar-39Ar analyses of a total of 26 samples from eight shock-darkened impact melt breccias of H-chondrite affinity (Gao-Guenie, LAP 02240, LAP 03922, LAP 031125, LAP 031173, LAP 031308, NWA 2058, and Ourique) are reported. These appear to record impacts ranging in time from 303 ± 56 Ma (Gao-Guenie) to 4360 ± 120 Ma (Ourique) ago. Three record impacts 300-400 Ma ago, while two others record impacts 3900-4000 Ma ago. Combining these with other impact ages from H chondrites in the literature, it appears that H chondrites record impacts in the first 100 Ma of solar system history, during the era of the "lunar cataclysm" and shortly thereafter (3500-4000 Ma ago), one or more impacts ∼300 Ma ago, and perhaps an impact ∼500 Ma ago (near the time of the L chondrite parent body disruption). Records of impacts on the H chondrite parent body are rare or absent between the era of planetary accretion and the "lunar cataclysm" (4400-4050 Ma), during the long stretch between heavy bombardment and recent breakup events (3500-1000 Ma), or at the time of final breakup into meteorite-sized bodies (<50 Ma).

Original languageEnglish (US)
Pages (from-to)747-762
Number of pages16
JournalMeteoritics and Planetary Science
Volume44
Issue number5
DOIs
Publication statusPublished - May 2009

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ASJC Scopus subject areas

  • Geophysics
  • Space and Planetary Science

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