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.2014 Jun;14(6):534-40.
doi: 10.1089/ast.2014.1150. Epub 2014 May 27.

Chance and necessity in biochemistry: implications for the search for extraterrestrial biomarkers in Earth-like environments

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Chance and necessity in biochemistry: implications for the search for extraterrestrial biomarkers in Earth-like environments

Alfonso F Davila et al. Astrobiology.2014 Jun.

Abstract

In this paper, we examine a restricted subset of the question of possible alien biochemistries. That is, we look into how different life might be if it emerged in environments similar to that required for life on Earth. We advocate a principle of chance and necessity in biochemistry. According to this principle, biochemistry is in some fundamental way the sum of two processes: there is an aspect of biochemistry that is an endowment from prebiotic processes, which represents the necessity, plus an aspect that is invented by the process of evolution, which represents the chance. As a result, we predict that life originating in extraterrestrial Earth-like environments will share biochemical motifs that can be traced back to the prebiotic world but will also have intrinsic biochemical traits that are unlikely to be duplicated elsewhere as they are combinatorially path-dependent. Effective and objective strategies to search for biomarkers, and evidence for a second genesis, on planets with Earth-like environments can be built based on this principle.

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Figures

<b>FIG. 1.</b>
FIG. 1.
Chance and necessity in biochemistry. Squares represent the chemical space occupied by a given biochemistry (e.g., Earth life, second genesis) as a function of molecule complexity (carbon number). The total chemical space is defined by the number of possible building blocks that are naturally available. Structurally and chemically simple building blocks (small carbon numbers) have a small number of possible isomers and therefore define a narrow chemical space. In addition, these simple building blocks are the most frequent and abundant in the prebiotic world. Hence, incipient life has few structural isomers to choose from, and these simple building blocks ought to be universal biochemical traits (prebiotic endowment ornecessity). As life evolves, the original set of building blocks is augmented by incorporation of more complex compounds. This expands the available chemical space—life has more structural isomers to choose from—and the probability that independent biochemistries choose the same building blocks decreases (evolutionary divergence orchance).
<b>FIG. 2.</b>
FIG. 2.
(A) Biochemical building blocks that could be common, if not universal, in Earth-like planets with life. These are the most frequent and abundant monomers in meteorites and in simulated prebiotic chemistry. (B) Examples of widespread biochemical traits in Earth life that were invented by the process of evolution and could be intrinsic to our planet only.
<b>FIG. 3.</b>
FIG. 3.
Differences in the frequency and relative abundances of the simplest α-amino acids found in meteorites (abiotic) and in different terrestrial samples (biogenic). While the same amino acids can be found in meteorites and in life, their relative abundances are different. Different patterns in the relative abundances of these prebiotically abundant building blocks could potentially be used as a biomarker. Amino acid concentrations in meteorites were obtained from Cronin and Pizzarello (1983), Ehrenfreundet al. (2001), and Martinset al. (2007). All other data were obtained from Aubrey (2008). Color images available online atwww.liebertonline.com/ast
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