Biological Homochirality and the Search for Extraterrestrial Biosignatures.

IF 1.9 4区 物理与天体物理 Q2 BIOLOGY
Marcelo Gleiser
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引用次数: 1

Abstract

Most amino acids and sugar molecules occur in mirror, or chiral, images of each other, knowns as enantiomers. However, life on Earth is mostly homochiral: proteins contain almost exclusively L-amino acids, while only D-sugars appear in RNA and DNA. The mechanism behind this fundamental asymmetry of life remains unknown, despite much progress in the theoretical and experimental understanding of homochirality in the past decades. We review three potential mechanisms for the emergence of biological homochirality on primal Earth and explore their implications for astrobiology: the first, that biological homochirality is a stochastic process driven by local environmental fluctuations; the second, that it is driven by circularly-polarized ultraviolet radiation in star-forming regions; and the third, that it is driven by parity violation at the elementary particle level. We argue that each of these mechanisms leads to different observational consequences for the existence of enantiomeric excesses in our solar system and in exoplanets, pointing to the possibility that the search for life elsewhere will help elucidate the origins of homochirality on Earth.

Abstract Image

生物同手性和寻找地外生物特征。
大多数氨基酸和糖分子互为镜像或手性映像,称为对映体。然而,地球上的生命大多是单手性的:蛋白质几乎只含有l -氨基酸,而RNA和DNA中只含有d -糖。尽管在过去的几十年里,对同手性的理论和实验理解取得了很大的进展,但这种基本的生命不对称性背后的机制仍然未知。我们回顾了原始地球上生物同手性出现的三种可能机制,并探讨了它们对天体生物学的影响:第一,生物同手性是一个由局部环境波动驱动的随机过程;第二,它是由恒星形成区域的圆偏振紫外线辐射驱动的;第三,它是由基本粒子层面的宇称破坏驱动的。我们认为,这些机制中的每一种都导致了太阳系和系外行星中对映体过量存在的不同观测结果,指出了在其他地方寻找生命将有助于阐明地球上同手性起源的可能性。
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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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