为 "生命 "下一个通用定义。

IF 1.9 4区 物理与天体物理 Q2 BIOLOGY
Marko Vitas, Andrej Dobovišek
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引用次数: 28

摘要

本文提出并讨论了生命的新定义。它是通过修改和扩展美国航天局的生命工作定义而提出的,该定义假定生命是一个 "能够进行达尔文进化的自我维持的化学系统"。新定义包括生命作为一个远离平衡系统的热力学方面,并考虑了从环境到生命系统的信息流。在推导生命定义的过程中,我们假定,在生命出现的过程中,进化必须首先涉及自催化系统,随后才获得遗传能力。新提出的生命定义与进化模式无关,无论拉马克进化论还是达尔文进化论在生命起源和整个进化历史中都起着作用。本文提出的生命新定义以最简约的方式表述,具有足够的概括性,不区分个体(新陈代谢)网络和集体(生态)网络。新提出的生命定义可能对天体生物学、生命起源研究或制造合成生命或人造生命的努力有意义,而且还可能对认知科学和计算机科学产生影响。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Towards a General Definition of Life.

A new definition of life is proposed and discussed in the present article. It is formulated by modifying and extending NASA's working definition of life, which postulates that life is a "self-sustaining chemical system capable of Darwinian evolution". The new definition includes a thermodynamical aspect of life as a far from equilibrium system and considers the flow of information from the environment to the living system. In our derivation of the definition of life we have assumed the hypothesis, that during the emergence of life evolution had to first involve autocatalytic systems that only subsequently acquired the capacity of genetic heredity. The new proposed definition of life is independent of the mode of evolution, regardless of whether Lamarckian or Darwinian evolution operated at the origins of life and throughout evolutionary history. The new definition of life presented herein is formulated in a minimal manner and it is general enough that it does not distinguish between individual (metabolic) network and the collective (ecological) one. The newly proposed definition of life may be of interest for astrobiology, research into the origins of life or for efforts to produce synthetic or artificial life, and it furthermore may also have implications in the cognitive and computer sciences.

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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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