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元古宙时期一氧化二氮和甲烷引起的温室效应。

Greenhouse warming by nitrous oxide and methane in the Proterozoic Eon.

机构信息

Department of Geosciences, Pennsylvania State University, University Park, PA, USA.

出版信息

Geobiology. 2011 Jul;9(4):313-20. doi: 10.1111/j.1472-4669.2011.00286.x.

Abstract

An anoxic, sulfidic ocean that may have existed during the Proterozoic Eon (0.54-2.4 Ga) would have had limited trace metal abundances because of the low solubility of metal sulfides. The lack of copper, in particular, could have had a significant impact on marine denitrification. Copper is needed for the enzyme that controls the final step of denitrification, from N(2) O to N(2) . Today, only about 5-6% of denitrification results in release of N(2) O. If all denitrification stopped at N(2) O during the Proterozoic, the N(2) O flux could have been 15-20 times higher than today, producing N(2) O concentrations of several ppmv, but only if O(2) levels were relatively high (>0.1 PAL). At lower O(2) levels, N(2) O is rapidly photodissociated. Methane concentrations may also have been elevated during this time, as has been previously suggested. A lack of dissolved O(2) and sulfate in the deep ocean could have produced a high methane flux from marine sediments, as much as 10-20 times today's methane flux from land. The photochemical lifetime of CH(4) increases as more CH(4) is added to the atmosphere, so CH(4) concentrations of up to 100 ppmv are possible during this time. The combined greenhouse effect of CH(4) and N(2) O could have provided up to 10° of warming, thereby keeping the surface warm during the Proterozoic without necessitating high CO(2) levels. A second oxygenation event near the end of the Proterozoic would have resulted in a reduction in both atmospheric N(2) O and CH(4) , perhaps triggering the Neoproterozoic "Snowball Earth" glaciations.

摘要

一个缺氧、硫化的海洋可能存在于元古代(0.54-2.4 Ga),由于金属硫化物的低溶解度,痕量金属的丰度会受到限制。特别是铜的缺乏可能对海洋反硝化作用产生重大影响。铜是控制反硝化作用最后一步的酶所必需的,从 N(2)O 到 N(2)。今天,只有大约 5-6%的反硝化作用导致 N(2)O 的释放。如果在元古代所有的反硝化作用都在 N(2)O 处停止,那么 N(2)O 的通量可能比今天高 15-20 倍,产生几个 ppmv 的 N(2)O 浓度,但前提是 O(2)水平相对较高(>0.1 PAL)。在较低的 O(2)水平下,N(2)O 会迅速光解。甲烷浓度也可能在这段时间内升高,正如之前所建议的那样。深海中缺乏溶解氧和硫酸盐可能导致从海洋沉积物中产生高甲烷通量,是今天从陆地产生的甲烷通量的 10-20 倍。随着大气中添加的 CH(4)增多,CH(4)的光化学寿命会增加,因此在这段时间内 CH(4)的浓度可能高达 100 ppmv。CH(4)和 N(2)O 的综合温室效应可能提供高达 10°的变暖,从而在元古代保持表面温暖,而无需高 CO(2)水平。元古代末期的第二次氧气化事件将导致大气 N(2)O 和 CH(4)的减少,可能引发新元古代的“雪球地球”冰川作用。

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