Decorated Vesicles as Prebiont Systems (a Hypothesis)

IF 1.9 4区 物理与天体物理 Q2 BIOLOGY
Martin Fisk, Radu Popa
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Abstract

Decorated vesicles in deep, seafloor basalts form abiotically, but show at least four life-analogous features, which makes them a candidate for origin of life research. These features are a physical enclosure, carbon-assimilatory catalysts, semi-permeable boundaries, and a source of usable energy. The nanometer-to-micron-sized spherules on the inner walls of decorated vesicles are proposed to function as mineral proto-enzymes. Chemically, these structures resemble synthetic FeS clusters shown to convert CO2, CO and H2 into methane, formate, and acetate. Secondary phyllosilicate minerals line the vesicles’ inner walls and can span openings in the vesicles and thus can act as molecular sieves between the vesicles’ interior and the surrounding aquifer. Lastly, basalt glass in the vesicle walls takes up protons, which replace cations in the silicate framework. This results in an inward proton flux, reciprocal outward flux of metal cations, more alkaline pH inside the vesicle than outside, and production of more phyllosilicates. Such life-like features could have been exploited to move decorated vesicles toward protolife systems. Decorated vesicles are proposed as study models of prebiotic systems that are expected to have existed on the early Earth and Earth-like exoplanets. Their analysis can lead to better understanding of changes in planetary geocycles during the origin of life.

Abstract Image

装饰囊泡是前生物系统(一种假设)
深海海底玄武岩中的装饰囊泡是非生物形成的,但至少显示出四个类似生命的特征,这使它们成为生命起源研究的候选对象。这些特征是物理封闭、碳同化催化剂、半渗透边界和可用能量来源。装饰囊泡内壁上的纳米到微米大小的球体被认为具有矿物原酶的功能。从化学角度看,这些结构类似于合成的 FeS 簇,可以将 CO2、CO 和 H2 转化为甲烷、甲酸盐和醋酸盐。次生植物硅酸盐矿物排列在囊泡内壁上,并能穿过囊泡的开口,因此可以充当囊泡内部和周围含水层之间的分子筛。最后,囊泡内壁的玄武岩玻璃吸收质子,取代硅酸盐框架中的阳离子。这导致质子向内流动,金属阳离子向外流动,囊泡内部的 pH 值比外部更偏碱性,并产生更多的植硅酸盐。这些类似生命的特征可能会被利用来推动装饰囊泡向原生生命系统发展。建议将装饰囊泡作为预计存在于早期地球和类地系外行星上的前生物系统的研究模型。对它们的分析有助于更好地理解生命起源过程中行星地球周期的变化。
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来源期刊
CiteScore
3.20
自引率
15.00%
发文量
12
审稿时长
>12 weeks
期刊介绍: The subject of the origin and early evolution of life is an inseparable part of the general discipline of Astrobiology. The journal Origins of Life and Evolution of Biospheres places special importance on the interconnection as well as the interdisciplinary nature of these fields, as is reflected in its subject coverage. While any scientific study which contributes to our understanding of the origins, evolution and distribution of life in the Universe is suitable for inclusion in the journal, some examples of important areas of interest are: prebiotic chemistry and the nature of Earth''s early environment, self-replicating and self-organizing systems, the theory of the RNA world and of other possible precursor systems, and the problem of the origin of the genetic code. Early evolution of life - as revealed by such techniques as the elucidation of biochemical pathways, molecular phylogeny, the study of Precambrian sediments and fossils and of major innovations in microbial evolution - forms a second focus. As a larger and more general context for these areas, Astrobiology refers to the origin and evolution of life in a cosmic setting, and includes interstellar chemistry, planetary atmospheres and habitable zones, the organic chemistry of comets, meteorites, asteroids and other small bodies, biological adaptation to extreme environments, life detection and related areas. Experimental papers, theoretical articles and authorative literature reviews are all appropriate forms for submission to the journal. In the coming years, Astrobiology will play an even greater role in defining the journal''s coverage and keeping Origins of Life and Evolution of Biospheres well-placed in this growing interdisciplinary field.
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