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深海沉积物中星际尘埃颗粒对太阳氦和氖的保留

Retention of Solar Helium and Neon in IDPs in Deep Sea Sediment.

作者信息

Hiyagon H

出版信息

Science. 1994 Mar 4;263(5151):1257-9. doi: 10.1126/science.263.5151.1257.

Abstract

It was recently proposed that subduction of interplanetary dust particles (IDPs) contained in deep sea sediments could have introduced substantial solar helium and neon to the Earth's mantle. However, it is not certain if IDPs would retain solar noble gases during subduction. A diffusion experiment that examined He and Ne in IDPs in a magnetic separate from Pacific Ocean sediments showed that He and Ne would be lost from IDPs within 3 years at 500 degrees C, and possibly within 10(5) years at 200 degrees C, which suggests that they would be lost from subducting slabs at shallow depths.

摘要

最近有人提出,深海沉积物中所含的行星际尘埃颗粒(IDP)的俯冲作用可能已将大量的太阳氦和氖引入了地球地幔。然而,尚不确定IDP在俯冲过程中是否会保留太阳惰性气体。一项在与太平洋沉积物分离的磁性环境中检测IDP中氦和氖的扩散实验表明,在500摄氏度下,氦和氖会在3年内从IDP中流失,在200摄氏度下可能在10^5年内流失,这表明它们会在浅深度的俯冲板块中流失。

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