Lunar impact history from 40Ar/39Ar dating of glass spherules

被引:155
作者
Culler, TS
Becker, TA
Muller, RA
Renne, PR [1 ]
机构
[1] Univ Calif Berkeley, Dept Geol & Geophys, Berkeley, CA 94720 USA
[2] Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA
[3] Univ Calif Berkeley, Lawrence Berkeley Lab, Berkeley, CA 94720 USA
[4] Berkeley Geochronol Ctr, Berkeley, CA 94709 USA
关键词
D O I
10.1126/science.287.5459.1785
中图分类号
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号
07 ; 0710 ; 09 ;
摘要
Lunar spherules are small glass beads that are formed mainly as a result of small impacts on the lunar surface; the ages of these impacts can be determined by the 40Ar/39Ar isochron technique. Here, 155 spherules separated from 1 gram of Apollo 14 soil were analyzed using this technique. The data show that over the Last similar to 3.5 billion years, the cratering rate decreased by a factor of 2 to 3 to a low about 500 to 600 million years ago, then increased by a factor of 3.7 +/- 1.2 in the last 400 million years. This latter period coincided with rapid biotic evolutionary radiation on Earth.
引用
收藏
页码:1785 / 1788
页数:4
相关论文
共 30 条
[11]  
GROTZINGER JP, 1997, AAPG BULL, V18, P1954
[12]  
Hartmann W.K., 1980, P C LUNAR HIGHLANDS, P155
[13]   PALEOCRATERING OF MOON - REVIEW OF POST-APOLLO DATA [J].
HARTMANN, WK .
ASTROPHYSICS AND SPACE SCIENCE, 1972, 17 (01) :48-&
[14]  
Heiken G. H., 1991, Lunar sourcebook
[15]  
Horz F, 1991, LUNAR SOURCEBOOK, P285
[16]   The Phanerozoic impact cratering rate: Evidence from the farside of the moon [J].
McEwen, AS ;
Moore, JM ;
Shoemaker, EM .
JOURNAL OF GEOPHYSICAL RESEARCH-PLANETS, 1997, 102 (E4) :9231-9242
[17]   EJECTA FROM LARGE CRATERS ON MOON - DISCUSSION [J].
SETTLE, M ;
HEAD, JW ;
MCGETCHI.TR .
EARTH AND PLANETARY SCIENCE LETTERS, 1974, 23 (03) :271-273
[18]  
MCKAY DS, 1973, EOS T AM GEOPHYS UN, V54, P599
[19]  
MORRIS RV, 1983, 19069 JSC LB JOHNS S
[20]  
MULLER RA, 1993, LBL34168 L BERK NAT