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An Astrophysical Basis for a Universal Origin of Life

机译:宇宙万物起源的天文学基础

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We propose a universal, astrophysically based theory of the origin of life on Earth and on other rocky planets as well. Life is an information system where the information content grows because of selection. It must start with the minimum possible information, or the minimum possible departure from thermodynamic equilibrium. It also requires thermodynamically free energy that is accessible by means of its information content. Hence, for its origin, we look for the most benign circumstance or minimum entropy variations over long times with abundant free energy. The unique location for this condition is the pore space in the first few kilometers of the earth's surface. The free energy is derived from the condensed products of the chemical reactions taking place in the cooling nebula e.g. iron oxides and fixed hydrocarbon, (CH_2)_(16) and the benign environment is the thermal and radiation isolation of the earth's crust. We discuss how this environment occurs naturally and universally astrophysically. We then propose several chemical routes to the formation of life with a minimum entropy departure from thermodynamic equilibrium.
机译:我们提出了一种基于天体物理学的普遍性理论,来研究地球以及其他岩石行星上的生命起源。生命是一个信息系统,信息内容因选择而增长。它必须以最小的可能信息或最小的热力学平衡开始。它还需要通过其信息内容可访问的热力学自由能。因此,对于它的起源,我们寻找具有丰富自由能的长期最佳状态或最小熵变化。这种情况的唯一位置是地球表面前几公里的孔隙空间。自由能是从冷却星云中发生的化学反应的冷凝产物中获得的。氧化铁和固定碳氢化合物(CH_2)_(16)和良性环境是地壳的热和辐射隔离。我们讨论了这种环境是如何自然发生的以及普遍存在于天体的。然后,我们提出了以最小的熵偏离热力学平衡的方式形成生命的几种化学途径。

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