TY - JOUR
T1 - 40Ar-39Ar ages of H-chondrite impact melt breccias
AU - Swindle, Timothy D.
AU - Isachsen, Clark E.
AU - Weirich, John R.
AU - Kring, David A.
PY - 2009/5
Y1 - 2009/5
N2 - 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).
AB - 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).
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U2 - 10.1111/j.1945-5100.2009.tb00766.x
DO - 10.1111/j.1945-5100.2009.tb00766.x
M3 - Article
AN - SCOPUS:69649106332
SN - 1086-9379
VL - 44
SP - 747
EP - 762
JO - Meteoritics and Planetary Science
JF - Meteoritics and Planetary Science
IS - 5
ER -