地球上的生命可以在地球外的有机碳上生长。

Life on Earth can grow on extraterrestrial organic carbon.

机构信息

UK Centre for Astrobiology, University of Edinburgh, Edinburgh, UK.

Centre for Metabolomics Research, Department of Biochemistry, Cell and Systems Biology, Institute of Systems, Molecular and Integrative Biology, University of Liverpool, Liverpool, UK.

出版信息

Sci Rep. 2024 Feb 14;14(1):3691. doi: 10.1038/s41598-024-54195-6.

Abstract

The universe is a vast store of organic abiotic carbon that could potentially drive heterotrophy on habitable planets. Meteorites are one of the transporters of this carbon to planetary surfaces. Meteoritic material was accumulating on early Earth when life emerged and proliferated. Yet it is not known if this organic carbon from space was accessible to life. In this research, an anaerobic microbial community was grown with the CM2 carbonaceous chondrite Aguas Zarcas as the sole carbon, energy and nutrient source. Using a reversed C-stable isotope labelling experiment in combination with optical photothermal infrared (O-PTIR) spectroscopy of single cells, this paper demonstrates the direct transfer of carbon from meteorite into microbial biomass. This implies that meteoritic organics could have been used as a carbon source on early Earth and other habitable planets, and supports the potential for a heterotrophic metabolism in early living systems.

摘要

宇宙是一个有机无生命碳的巨大储存库,它有可能为可居住行星上的异养生物提供动力。陨石是将这种碳输送到行星表面的载体之一。当生命出现并繁衍时,陨石物质正在早期地球上积累。然而,目前尚不清楚来自太空的这种有机碳是否可供生命利用。在这项研究中,一种厌氧微生物群落以 CM2 碳质球粒陨石 Aguas Zarcas 作为唯一的碳、能源和营养来源进行培养。本文利用反向 C 稳定同位素标记实验与单细胞光学光热红外(O-PTIR)光谱相结合,证明了碳从陨石直接转移到微生物生物量中。这意味着陨石有机物可能曾被用作早期地球上和其他可居住行星上的碳源,并支持早期生命系统中存在异养代谢的可能性。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/3305/10866878/4d287a93e742/41598_2024_54195_Fig1_HTML.jpg

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