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本文引用的文献

1
Earth's earliest atmospheres.地球早期的大气。
Cold Spring Harb Perspect Biol. 2010 Oct;2(10):a004895. doi: 10.1101/cshperspect.a004895. Epub 2010 Jun 23.
2
Cosmic carbon chemistry: from the interstellar medium to the early Earth.宇宙碳化学:从星际介质到早期地球。
Cold Spring Harb Perspect Biol. 2010 Dec;2(12):a002097. doi: 10.1101/cshperspect.a002097. Epub 2010 Jun 16.
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Planetary organic chemistry and the origins of biomolecules.行星有机化学与生物分子起源。
Cold Spring Harb Perspect Biol. 2010 Jul;2(7):a003467. doi: 10.1101/cshperspect.a003467. Epub 2010 May 26.
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Mineral surfaces, geochemical complexities, and the origins of life.矿物表面、地球化学复杂性与生命起源。
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An origin of life on Mars.火星上的生命起源。
Cold Spring Harb Perspect Biol. 2010 Apr;2(4):a003509. doi: 10.1101/cshperspect.a003509. Epub 2010 Mar 3.
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Bioenergetics and life's origins.生物能量学与生命起源。
Cold Spring Harb Perspect Biol. 2010 Feb;2(2):a004929. doi: 10.1101/cshperspect.a004929.
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Deep phylogeny--how a tree can help characterize early life on Earth.深度系统发育——一棵树如何帮助描绘地球上的早期生命。
Cold Spring Harb Perspect Biol. 2010 Jan;2(1):a002238. doi: 10.1101/cshperspect.a002238.
8
Timing of morphological and ecological innovations in the cyanobacteria--a key to understanding the rise in atmospheric oxygen.蓝细菌形态和生态创新的时间——理解大气氧气增加的关键。
Geobiology. 2010 Jan;8(1):1-23. doi: 10.1111/j.1472-4669.2009.00220.x. Epub 2009 Oct 23.
9
(142)Nd evidence for an enriched Hadean reservoir in cratonic roots.克拉通根中存在富集冥古宙储层的证据(142)。
Nature. 2009 Jun 25;459(7250):1118-21. doi: 10.1038/nature08089.
10
Low heat flow inferred from >4 Gyr zircons suggests Hadean plate boundary interactions.从年龄大于40亿年的锆石推断出的低热流表明冥古宙板块边界相互作用。
Nature. 2008 Nov 27;456(7221):493-6. doi: 10.1038/nature07465.

冥古宙-太古宙环境。

The Hadean-Archaean environment.

机构信息

Department of Geophysics, Stanford University, Stanford, CA 94305, USA.

出版信息

Cold Spring Harb Perspect Biol. 2010 Jun;2(6):a002527. doi: 10.1101/cshperspect.a002527. Epub 2010 May 5.

DOI:10.1101/cshperspect.a002527
PMID:20516134
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC2869525/
Abstract

A sparse geological record combined with physics and molecular phylogeny constrains the environmental conditions on the early Earth. The Earth began hot after the moon-forming impact and cooled to the point where liquid water was present in approximately 10 million years. Subsequently, a few asteroid impacts may have briefly heated surface environments, leaving only thermophile survivors in kilometer-deep rocks. A warm 500 K, 100 bar CO(2) greenhouse persisted until subducted oceanic crust sequestered CO(2) into the mantle. It is not known whether the Earth's surface lingered in a approximately 70 degrees C thermophile environment well into the Archaean or cooled to clement or freezing conditions in the Hadean. Recently discovered approximately 4.3 Ga rocks near Hudson Bay may have formed during the warm greenhouse. Alkalic rocks in India indicate carbonate subduction by 4.26 Ga. The presence of 3.8 Ga black shales in Greenland indicates that S-based photosynthesis had evolved in the oceans and likely Fe-based photosynthesis and efficient chemical weathering on land. Overall, mantle derived rocks, especially kimberlites and similar CO(2)-rich magmas, preserve evidence of subducted upper oceanic crust, ancient surface environments, and biosignatures of photosynthesis.

摘要

一个稀疏的地质记录,加上物理和分子系统发育学,限制了早期地球上的环境条件。月球形成的撞击使地球开始变得炽热,然后冷却,大约在 1000 万年内出现了液态水。随后,一些小行星撞击可能短暂地加热了地表环境,只留下在数公里深的岩石中生存的嗜热生物。一个温暖的 500K、100 巴 CO2 温室持续存在,直到俯冲的海洋地壳将 CO2 隔离到地幔中。目前尚不清楚地球表面是否在古生代时期长期处于约 70°C 的嗜热环境中,或者在冥古宙时期冷却到宜人或冰冻的条件。最近在哈德逊湾附近发现的大约 43 亿年前的岩石可能是在温暖的温室环境中形成的。印度的碱性岩石表明碳酸盐俯冲发生在 42.6 亿年前。格陵兰岛的 38 亿年前的黑色页岩的存在表明,S 基光合作用已经在海洋中进化,并且可能在陆地上发生了 Fe 基光合作用和有效的化学风化作用。总的来说,地幔来源的岩石,特别是金伯利岩和类似的富含 CO2 的岩浆,保存了俯冲的上层海洋地壳、古代地表环境和光合作用生物特征的证据。