陨石
小行星
天体生物学
喷出物
碰撞
火星探测计划
事件(粒子物理)
撞击坑
地质学
土(古典元素)
地球科学
物理
天文
天体物理学
计算机科学
超新星
计算机安全
作者
W. F. Bottke,David Vokrouhlický,S. Marchi,T. D. Swindle,E. R. D. Scott,J. R. Weirich,Harold F. Levison
出处
期刊:Science
[American Association for the Advancement of Science (AAAS)]
日期:2015-04-16
卷期号:348 (6232): 321-323
被引量:110
标识
DOI:10.1126/science.aaa0602
摘要
Traces of collisions within collisions The Moon is widely accepted to have been created by the collision of a Mars-sized body with Earth. However, information about exactly when this event occurred is still welcome. To find out more, Bottke et al. compared models and the meteorite record with estimates of impact heating. When ejecta was thrown off during the main collision, high-velocity kilometer-sized fragments hit and heated main-belt asteroids. Evidence of such collisions emerges when pieces of those asteroids turn up as meteorites on Earth. The model and empirical record converge on 4.48 billion years ago, confirming previous estimates reached by different approaches. Science , this issue p. 321
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