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      Systems protobiology: origin of life in lipid catalytic networks

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          Abstract

          Life is that which replicates and evolves, but there is no consensus on how life emerged. We advocate a systems protobiology view, whereby the first replicators were assemblies of spontaneously accreting, heterogeneous and mostly non-canonical amphiphiles. This view is substantiated by rigorous chemical kinetics simulations of the graded autocatalysis replication domain (GARD) model, based on the notion that the replication or reproduction of compositional information predated that of sequence information. GARD reveals the emergence of privileged non-equilibrium assemblies (composomes), which portray catalysis-based homeostatic (concentration-preserving) growth. Such a process, along with occasional assembly fission, embodies cell-like reproduction. GARD pre-RNA evolution is evidenced in the selection of different composomes within a sparse fitness landscape, in response to environmental chemical changes. These observations refute claims that GARD assemblies (or other mutually catalytic networks in the metabolism first scenario) cannot evolve. Composomes represent both a genotype and a selectable phenotype, anteceding present-day biology in which the two are mostly separated. Detailed GARD analyses show attractor-like transitions from random assemblies to self-organized composomes, with negative entropy change, thus establishing composomes as dissipative systems—hallmarks of life. We show a preliminary new version of our model, metabolic GARD (M-GARD), in which lipid covalent modifications are orchestrated by non-enzymatic lipid catalysts, themselves compositionally reproduced. M-GARD fills the gap of the lack of true metabolism in basic GARD, and is rewardingly supported by a published experimental instance of a lipid-based mutually catalytic network. Anticipating near-future far-reaching progress of molecular dynamics, M-GARD is slated to quantitatively depict elaborate protocells, with orchestrated reproduction of both lipid bilayer and lumenal content. Finally, a GARD analysis in a whole-planet context offers the potential for estimating the probability of life's emergence. The invigorated GARD scrutiny presented in this review enhances the validity of autocatalytic sets as a bona fide early evolution scenario and provides essential infrastructure for a paradigm shift towards a systems protobiology view of life's origin.

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          Visible light photoredox catalysis with transition metal complexes: applications in organic synthesis.

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            Hydrothermal vents and the origin of life.

            Submarine hydrothermal vents are geochemically reactive habitats that harbour rich microbial communities. There are striking parallels between the chemistry of the H(2)-CO(2) redox couple that is present in hydrothermal systems and the core energy metabolic reactions of some modern prokaryotic autotrophs. The biochemistry of these autotrophs might, in turn, harbour clues about the kinds of reactions that initiated the chemistry of life. Hydrothermal vents thus unite microbiology and geology to breathe new life into research into one of biology's most important questions - what is the origin of life?
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              Endogenous production, exogenous delivery and impact-shock synthesis of organic molecules: an inventory for the origins of life.

              Sources of organic molecules on the early Earth divide into three categories: delivery by extraterrestrial objects; organic synthesis driven by impact shocks; and organic synthesis by other energy sources (such as ultraviolet light or electrical discharges). Estimates of these sources for plausible end-member oxidation states of the early terrestrial atmosphere suggest that the heavy bombardment before 3.5 Gyr ago either produced or delivered quantities of organics comparable to those produced by other energy sources. Which sources of prebiotic organics were quantitatively dominant depends strongly on the composition of the early terrestrial atmosphere. In the event of an early strongly reducing atmosphere, production by atmospheric shocks seems to have dominated that due to electrical discharges. Organic synthesis by ultraviolet light may, in turn, have dominated shock production, but only if a long-wavelength absorber such as H2S were supplied to the atmosphere at a rate sufficient for synthesis to have been limited by ultraviolet flux, rather than by reactant abundance. In the apparently more likely case of an early terrestrial atmosphere of intermediate oxidation state, atmospheric shocks were probably of little importance for direct organic production. For [H2]/[CO2] ratios of approximately 0.1, net organic production was some three orders of magnitude lower than for reducing atmospheres, with delivery of intact exogenous organics in interplanetary dust particles (IDPs) and ultraviolet production being the most important sources. At still lower [H2]/[CO2] ratios, IDPs may have been the dominant source of prebiotic organics on the early Earth. Endogenous, exogenous and impact-shock sources of organics could each have made a significant contribution to the origins of life.
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                Author and article information

                Journal
                J R Soc Interface
                J R Soc Interface
                RSIF
                royinterface
                Journal of the Royal Society Interface
                The Royal Society
                1742-5689
                1742-5662
                July 2018
                25 July 2018
                25 July 2018
                : 15
                : 144
                : 20180159
                Affiliations
                [1 ]Department of Molecular Genetics, Weizmann Institute of Science , Rehovot 76100, Israel
                [2 ]Department of Molecular, Cell and Systems Biology, University of California , Riverside, CA 92521, USA
                [3 ]Origins Center, Center for Systems Chemistry, Stratingh Institute for Chemistry, University of Groningen , Groningen, the Netherlands
                [4 ]Blue Marble Space Institute of Science , Seattle, WA, USA
                Author notes
                Author information
                http://orcid.org/0000-0001-5424-1393
                http://orcid.org/0000-0003-0102-0196
                http://orcid.org/0000-0002-9706-5323
                Article
                rsif20180159
                10.1098/rsif.2018.0159
                6073634
                30045888
                7b048ea2-52a9-4a2a-945a-d88e084d9edb
                © 2018 The Authors.

                Published by the Royal Society under the terms of the Creative Commons Attribution License http://creativecommons.org/licenses/by/4.0/, which permits unrestricted use, provided the original author and source are credited.

                History
                : 6 March 2018
                : 29 June 2018
                Funding
                Funded by: CMST COST Action;
                Award ID: CM1304
                Funded by: The Crwon Huamn Genome Center at the Weizmann Institute of Science;
                Funded by: Minerva Center for Life under Extreme Planetary Conditions at the Weizmann Institute of Science;
                Funded by: NWA StartImpuls;
                Funded by: Morris Belkin Visiting Professorship at the Weizmann Institute of Science;
                Categories
                1004
                8
                70
                181
                Review Articles
                Review Article
                Custom metadata
                July, 2018

                Life sciences
                origin of life,prebiotic evolution,reflexively autocatalytic sets,composome networks,metabolism first,pre-rna world

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