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富含锌和钾的冥古宙寒冷地热场中RNA世界的起源:月球形成撞击产生的正向影响导致的自然发生?

Origin of the RNA World in Cold Hadean Geothermal Fields Enriched in Zinc and Potassium: Abiogenesis as a Positive Fallout from the Moon-Forming Impact?

作者信息

Mulkidjanian Armen Y, Dibrova Daria V, Bychkov Andrey Y

机构信息

Department of Physics, Osnabrueck University, D-49069 Osnabrueck, Germany.

Center of Cellular Nanoanalytics, Osnabrueck University, D-49069 Osnabrueck, Germany.

出版信息

Life (Basel). 2025 Mar 4;15(3):399. doi: 10.3390/life15030399.

DOI:10.3390/life15030399
PMID:40141744
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC11943819/
Abstract

The ubiquitous, evolutionarily oldest RNAs and proteins exclusively use rather rare zinc as transition metal cofactor and potassium as alkali metal cofactor, which implies their abundance in the habitats of the first organisms. Intriguingly, lunar rocks contain a hundred times less zinc and ten times less potassium than the Earth's crust; the Moon is also depleted in other moderately volatile elements (MVEs). Current theories of impact formation of the Moon attribute this depletion to the MVEs still being in a gaseous state when the hot post-impact disk contracted and separated from the nascent Moon. The MVEs then fell out onto juvenile Earth's protocrust; zinc, as the most volatile metal, precipitated last, just after potassium. According to our calculations, the top layer of the protocrust must have contained up to 10 kg of metallic zinc, a powerful reductant. The venting of hot geothermal fluids through this MVE-fallout layer, rich in metallic zinc and radioactive potassium, both capable of reducing carbon dioxide and dinitrogen, must have yielded a plethora of organic molecules released with the geothermal vapor. In the pools of vapor condensate, the RNA-like molecules may have emerged through a pre-Darwinian selection for low-volatile, associative, mineral-affine, radiation-resistant, nitrogen-rich, and polymerizable molecules.

摘要

无处不在且在进化上最古老的RNA和蛋白质仅使用相当稀有的锌作为过渡金属辅因子,使用钾作为碱金属辅因子,这意味着它们在最早生物的栖息地中含量丰富。有趣的是,月球岩石中的锌含量比地壳少一百倍,钾含量比地壳少十倍;月球中的其他中度挥发性元素(MVE)也很匮乏。目前关于月球撞击形成的理论将这种匮乏归因于在撞击后形成的热盘收缩并与新生月球分离时,中度挥发性元素仍处于气态。然后,这些中度挥发性元素落到了幼年地球的原始地壳上;锌作为挥发性最强的金属,在钾之后最后沉淀。根据我们的计算,原始地壳的顶层必定含有多达10千克的金属锌,这是一种强大的还原剂。通过富含金属锌和放射性钾的中度挥发性元素沉降层排放热的地热流体,这两种物质都能够还原二氧化碳和氮气,必定产生了大量随地热蒸汽释放的有机分子。在蒸汽凝结池中,类似RNA的分子可能是通过对低挥发性、缔合性、亲矿物性、抗辐射、富氮且可聚合的分子进行达尔文之前的选择而出现的。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/4452/11943819/1f6c6ed472da/life-15-00399-g006.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/4452/11943819/899bce11e6a1/life-15-00399-g001.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/4452/11943819/adad98244951/life-15-00399-g002.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/4452/11943819/536d57deac7d/life-15-00399-g003.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/4452/11943819/1f60a7133144/life-15-00399-g004.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/4452/11943819/87da6c959cee/life-15-00399-g005.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/4452/11943819/1f6c6ed472da/life-15-00399-g006.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/4452/11943819/899bce11e6a1/life-15-00399-g001.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/4452/11943819/adad98244951/life-15-00399-g002.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/4452/11943819/536d57deac7d/life-15-00399-g003.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/4452/11943819/1f60a7133144/life-15-00399-g004.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/4452/11943819/87da6c959cee/life-15-00399-g005.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/4452/11943819/1f6c6ed472da/life-15-00399-g006.jpg

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