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      Deciphering Biosignatures in Planetary Contexts

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          Abstract

          Microbial life permeates Earth's critical zone and has likely inhabited nearly all our planet's surface and near subsurface since before the beginning of the sedimentary rock record. Given the vast time that Earth has been teeming with life, do astrobiologists truly understand what geological features untouched by biological processes would look like? In the search for extraterrestrial life in the Universe, it is critical to determine what constitutes a biosignature across multiple scales, and how this compares with “abiosignatures” formed by nonliving processes. Developing standards for abiotic and biotic characteristics would provide quantitative metrics for comparison across different data types and observational time frames. The evidence for life detection falls into three categories of biosignatures: (1) substances, such as elemental abundances, isotopes, molecules, allotropes, enantiomers, minerals, and their associated properties; (2) objects that are physical features such as mats, fossils including trace-fossils and microbialites (stromatolites), and concretions; and (3) patterns, such as physical three-dimensional or conceptual n-dimensional relationships of physical or chemical phenomena, including patterns of intermolecular abundances of organic homologues, and patterns of stable isotopic abundances between and within compounds. Five key challenges that warrant future exploration by the astrobiology community include the following: (1) examining phenomena at the “right” spatial scales because biosignatures may elude us if not examined with the appropriate instrumentation or modeling approach at that specific scale; (2) identifying the precise context across multiple spatial and temporal scales to understand how tangible biosignatures may or may not be preserved; (3) increasing capability to mine big data sets to reveal relationships, for example, how Earth's mineral diversity may have evolved in conjunction with life; (4) leveraging cyberinfrastructure for data management of biosignature types, characteristics, and classifications; and (5) using three-dimensional to n-D representations of biotic and abiotic models overlain on multiple overlapping spatial and temporal relationships to provide new insights.

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          Most cited references269

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          Photocatalytic Reduction of CO2on TiO2and Other Semiconductors

          Rising atmospheric levels of carbon dioxide and the depletion of fossil fuel reserves raise serious concerns about the ensuing effects on the global climate and future energy supply. Utilizing the abundant solar energy to convert CO2 into fuels such as methane or methanol could address both problems simultaneously as well as provide a convenient means of energy storage. In this Review, current approaches for the heterogeneous photocatalytic reduction of CO2 on TiO2 and other metal oxide, oxynitride, sulfide, and phosphide semiconductors are presented. Research in this field is focused primarily on the development of novel nanostructured photocatalytic materials and on the investigation of the mechanism of the process, from light absorption through charge separation and transport to CO2 reduction pathways. The measures used to quantify the efficiency of the process are also discussed in detail.
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            Soft lithography in biology and biochemistry.

            Soft lithography, a set of techniques for microfabrication, is based on printing and molding using elastomeric stamps with the patterns of interest in basrelief. As a technique for fabricating microstructures for biological applications, soft lithography overcomes many of the shortcomings of photolithography. In particular, soft lithography offers the ability to control the molecular structure of surfaces and to pattern the complex molecules relevant to biology, to fabricate channel structures appropriate for microfluidics, and to pattern and manipulate cells. For the relatively large feature sizes used in biology (> or = 50 microns), production of prototype patterns and structures is convenient, inexpensive, and rapid. Self-assembled monolayers of alkanethiolates on gold are particularly easy to pattern by soft lithography, and they provide exquisite control over surface biochemistry.
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              Atmospheric influence of Earth's earliest sulfur cycle

              Mass-independent isotopic signatures for delta(33)S, delta(34)S, and delta(36)S from sulfide and sulfate in Precambrian rocks indicate that a change occurred in the sulfur cycle between 2090 and 2450 million years ago (Ma). Before 2450 Ma, the cycle was influenced by gas-phase atmospheric reactions. These atmospheric reactions also played a role in determining the oxidation state of sulfur, implying that atmospheric oxygen partial pressures were low and that the roles of oxidative weathering and of microbial oxidation and reduction of sulfur were minimal. Atmospheric fractionation processes should be considered in the use of sulfur isotopes to study the onset and consequences of microbial fractionation processes in Earth's early history.
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                Author and article information

                Journal
                Astrobiology
                Astrobiology
                ast
                Astrobiology
                Mary Ann Liebert, Inc., publishers (140 Huguenot Street, 3rd FloorNew Rochelle, NY 10801USA )
                1531-1074
                1557-8070
                01 September 2019
                22 August 2019
                22 August 2019
                : 19
                : 9
                : 1075-1102
                Affiliations
                [ 1 ]Department of Geology & Geophysics, University of Utah, Salt Lake City, Utah.
                [ 2 ]Department of Geosciences, University of Montana, Missoula, Montana.
                [ 3 ]Geology Department, Southern Illinois University, Carbondale, Illinois.
                [ 4 ]Department of Electrical and Computer Engineering, Baylor University, Waco, Texas.
                [ 5 ]Earth-Life Science Institute, Tokyo Institute of Technology, Tokyo, Japan.
                [ 6 ]Electronics and Computer Science, Institute for Life Sciences, University of Southampton, Southampton, United Kingdom.
                [ 7 ]Department of Earth Science, University of California, Santa Barbara, Santa Barbara, California.
                [ 8 ]NASA Astrobiology Institute, NASA Ames Research Center, Moffett Field, California.
                [ 9 ]Department of Astronomy, University of Maryland College Park (CRESST), College Park, Maryland.
                [ 10 ]NASA Goddard Space Flight Center, Greenbelt, Maryland.
                [ 11 ]Exobiology Branch, NASA Ames Research Center, Moffett Field, Californnia.
                [ 12 ]School of Earth and Space Exploration, Arizona State University, Tempe, Arizona.
                [ 13 ]Research School of Earth Sciences, The Australian National University, Canberra, Australia.
                [ 14 ]Geophysical Laboratory, Carnegie Institution for Science, Washington, District of Columbia.
                [ 15 ]Department of Earth and Planetary Sciences, McGill University, Montreal, Canada.
                [ 16 ]Geosciences Department, John Abbott College, Sainte-Anne-de-Bellevue, Canada.
                [ 17 ]London Centre for Nanotechnology, University College London, London, United Kingdom.
                [ 18 ]Department of Earth Sciences, University College London, London, United Kingdom.
                [ 19 ]Centre for Planetary Sciences, University College London, London, United Kingdom.
                [ 20 ]BioGeology and Environmental Geology State Key Laboratory, School of Earth Sciences, China University of Geosciences, Wuhan, China.
                [ 21 ]Department of Geological Sciences, University of Colorado Boulder, Boulder, Colorado.
                [ 22 ]Earth Sciences Department, Vrije Universiteit Amsterdam, Amsterdam, The Netherlands.
                [ 23 ]Department of Civil and Environmental Engineering, Colorado School of Mines, Golden, Colorado.
                [ 24 ]School of Earth and Environmental Sciences, The University of Queensland, St. Lucia, Queensland, Australia.
                [ 25 ]Program in Interdisciplinary Studies, Institute for Advanced Study, Princeton, New Jersey.
                Author notes
                [*]Address correspondence to: Marjorie A. Chan, Department of Geology & Geophysics, University of Utah, 115 S. 1460 E., Salt Lake City, UT 84112 marjorie.chan@ 123456utah.edu
                Article
                10.1089/ast.2018.1903
                10.1089/ast.2018.1903
                6708275
                31335163
                355e18ce-5d94-4b37-9ab6-196290d82aa4
                © Marjorie A. Chan et al., 2019; Published by Mary Ann Liebert, Inc.

                This Open Access article is distributed under the terms of the Creative Commons License ( http://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly credited.

                History
                : 14 May 2018
                : 10 March 2019
                Page count
                Figures: 11, Tables: 1, References: 260, Pages: 28
                Categories
                Review Article

                astrobiology,biosignatures,taphonomy,extraterrestrial life,extremophile.

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