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太阳系内部生命形成挥发元素的起源。

Origin of life-forming volatile elements in the inner Solar System.

机构信息

Université de Lorraine, CNRS, CRPG, Nancy, France.

Woods Hole Oceanographic Institution, Woods Hole, MA, USA.

出版信息

Nature. 2022 Nov;611(7935):245-255. doi: 10.1038/s41586-022-05276-x. Epub 2022 Nov 9.

Abstract

Volatile elements such as hydrogen, carbon, nitrogen and oxygen are essential ingredients to build habitable worlds like Earth, but their origin and evolution on terrestrial planets remain highly debated. Here we discuss the processes that distributed these elements throughout the early Solar System and how they then became incorporated into planetary building blocks. Volatiles on Earth and the other terrestrial planets appear to have been heterogeneously sourced from different Solar System reservoirs. The sources of planetary volatiles and the timing at which they were accreted to growing planets probably play a crucial role in controlling planet habitability.

摘要

挥发性元素,如氢、碳、氮和氧,是构建类地行星的必要成分,如地球,但它们在类地行星上的起源和演化仍然存在很大争议。在这里,我们讨论了将这些元素分布到整个早期太阳系的过程,以及它们后来是如何成为行星组成部分的。地球和其他类地行星上的挥发物似乎是从太阳系不同的储库中不均匀地产生的。行星挥发物的来源以及它们被吸积到生长行星上的时间,可能在控制行星宜居性方面起着至关重要的作用。

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