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月球土壤中的陆地氮和稀有气体。

Terrestrial nitrogen and noble gases in lunar soils.

作者信息

Ozima M, Seki K, Terada N, Miura Y N, Podosek F A, Shinagawa H

机构信息

Graduate School of Earth and Planetary Science, University of Tokyo, Tokyo 113-0033, Japan.

出版信息

Nature. 2005 Aug 4;436(7051):655-9. doi: 10.1038/nature03929.

Abstract

The nitrogen in lunar soils is correlated to the surface and therefore clearly implanted from outside. The straightforward interpretation is that the nitrogen is implanted by the solar wind, but this explanation has difficulties accounting for both the abundance of nitrogen and a variation of the order of 30 per cent in the 15N/14N ratio. Here we propose that most of the nitrogen and some of the other volatile elements in lunar soils may actually have come from the Earth's atmosphere rather than the solar wind. We infer that this hypothesis is quantitatively reasonable if the escape of atmospheric gases, and implantation into lunar soil grains, occurred at a time when the Earth had essentially no geomagnetic field. Thus, evidence preserved in lunar soils might be useful in constraining when the geomagnetic field first appeared. This hypothesis could be tested by examination of lunar farside soils, which should lack the terrestrial component.

摘要

月球土壤中的氮与表面相关,因此显然是从外部注入的。直接的解释是氮是由太阳风注入的,但这种解释难以说明氮的丰度以及15N/14N比值中30%左右的变化。在此我们提出,月球土壤中的大部分氮和一些其他挥发性元素实际上可能来自地球大气层而非太阳风。我们推断,如果大气气体的逸出以及向月球土壤颗粒中的注入发生在地球基本没有地磁场的时候,那么这个假设在数量上是合理的。因此,保存在月球土壤中的证据可能有助于确定地磁场首次出现的时间。这个假设可以通过检查月球背面的土壤来验证,因为背面的土壤应该没有地球成分。

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