Accretion rates of meteorites and cosmic dust in the Early Ordovician

被引:65
作者
Schmitz, B
PeuckerEhrenbrink, E
Lindstrom, M
Tassinari, M
机构
[1] WOODS HOLE OCEANOG INST,DEPT MARINE CHEM & GEOCHEM,WOODS HOLE,MA 02543
[2] UNIV STOCKHOLM,DEPT GEOL & GEOCHEM,S-10691 STOCKHOLM,SWEDEN
[3] PALEO GEOL CTR,S-53130 LINKOPING,SWEDEN
关键词
D O I
10.1126/science.278.5335.88
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
Abundant fossil meteorites in marine, condensed Lower Ordovician limestones from Kinnekulle, Sweden, indicate that accretion rates of meteorites were one to two orders of magnitude higher during an interval of the Early Ordovician than at0 present, Osmium isotope and iridium analyses of whole-rock limestone indicate a coeval enhancement of one order of magnitude in the influx rate of cosmic dust. Enhanced accretion of cosmic matter may be related to the disruption of the L chondrite parent body around 500 million years ago.
引用
收藏
页码:88 / 90
页数:3
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