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始新世晚期彗星雨的地球化学证据。

Geochemical evidence for a comet shower in the late Eocene.

作者信息

Farley K A, Montanari A, Shoemaker E M, Shoemaker C S

机构信息

Division of Geological and Planetary Sciences, California Institute of Technology, MS 170-25, Pasadena, CA 91125, USA.

出版信息

Science. 1998 May 22;280(5367):1250-3. doi: 10.1126/science.280.5367.1250.

Abstract

Analyses of pelagic limestones indicate that the flux of extraterrestrial helium-3 to Earth was increased for a 2.5-million year (My) period in the late Eocene. The enhancement began approximately 1 My before and ended approximately 1.5 My after the major impact events that produced the large Popigai and Chesapeake Bay craters approximately 36 million years ago. The correlation between increased concentrations of helium-3, a tracer of fine-grained interplanetary dust, and large impacts indicates that the abundance of Earth-crossing objects and dustiness in the inner solar system were simultaneously but only briefly enhanced. These observations provide evidence for a comet shower triggered by an impulsive perturbation of the Oort cloud.

摘要

远洋石灰岩分析表明,在始新世晚期的250万年时间里,地球的外星氦-3通量有所增加。这种增强在大约3600万年前形成大型波皮盖和切萨皮克湾陨石坑的重大撞击事件之前约100万年开始,在该事件之后约150万年结束。氦-3(细粒行星际尘埃的一种示踪剂)浓度增加与大型撞击之间的相关性表明,内太阳系中穿越地球物体的丰度和尘埃度同时但只是短暂增强。这些观测结果为奥尔特云的脉冲扰动引发彗星雨提供了证据。

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