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Science 1 December 2000: Vol. 290. no. 5497, pp. 1754 - 1756 DOI: 10.1126/science.290.5497.1754
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Reports
Support for the Lunar Cataclysm Hypothesis from Lunar Meteorite Impact Melt Ages
B. A. Cohen,*
T. D. Swindle,
D. A. Kring
Lunar meteorites represent a more random sampling of
lunar material than the Apollo or Luna collections and, as such, lunar meteorite impact melt ages are the most important data in nearly 30 years with which to reexamine the lunar cataclysm hypothesis. Within
the lunar meteorite breccias MAC 88105, QUE 93069, DaG 262, and DaG
400, seven to nine different impact events are represented with
40Ar-39Ar ages between 2.76 and 3.92 billion
years ago (Ga). The lack of impact melt older than 3.92 Ga supports the
concept of a short, intense period of bombardment in the Earth-moon
system at ~3.9 Ga. This was an anomalous spike of impact activity on
the otherwise declining impact- frequency curve.
The University of Arizona, Tucson, AZ 85721, USA.
*
Present address: Department of Geological Sciences, University
of Tennessee, Knoxville, TN 37996, USA.
To whom correspondence should be addressed. E-mail:
bcohen{at}utk.edu
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