Massive impact-induced release of carbon and sulfur gases in the early Earth's atmosphere

被引:13
|
作者
Marchi, S. [1 ]
Black, B. A. [2 ]
Elkins-Tanton, L. T. [3 ]
Bottke, W. F. [1 ]
机构
[1] Southwest Res Inst, Boulder, CO 80309 USA
[2] CUNY, City Coll, New York, NY 10021 USA
[3] Arizona State Univ, Tempe, AZ USA
关键词
early earth; asteroid impacts; faint young Sun; earth's atmosphere; CONTINENTAL-CRUST; OXIDATION-STATE; ISOTOPIC EVIDENCE; ASTEROID IMPACTS; DETRITAL ZIRCONS; MIDOCEAN RIDGES; OCEAN-RIDGE; CO2; MANTLE; DIOXIDE;
D O I
10.1016/j.epsl.2016.05.032
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
Recent revisions to our understanding of the collisional history of the Hadean and early-Archean Earth indicate that large collisions may have been an important geophysical process. In this work we show that the early bombardment flux of large impactors (>100 km) facilitated the atmospheric release of greenhouse gases (particularly CO2) from Earth's mantle. Depending on the timescale for the drawdown of atmospheric CO2, the Earth's surface could have been subject to prolonged clement surface conditions or multiple freeze-thaw cycles. The bombardment also delivered and redistributed to the surface large quantities of sulfur, one of the most important elements for life. The stochastic occurrence of large collisions could provide insights on why the Earth and Venus, considered Earth's twin planet, exhibit radically different atmospheres. (C) 2016 Elsevier B.V. All rights reserved.
引用
收藏
页码:96 / 104
页数:9
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