TY - JOUR
T1 - Deciphering Biosignatures in Planetary Contexts
AU - Chan, Marjorie A.
AU - Hinman, Nancy W.
AU - Potter-Mcintyre, Sally L.
AU - Schubert, Keith E.
AU - Gillams, Richard J.
AU - Awramik, Stanley M.
AU - Boston, Penelope J.
AU - Bower, Dina M.
AU - Des Marais, David J.
AU - Farmer, Jack
AU - Jia, Tony Z.
AU - King, Penelope L.
AU - Hazen, Robert M.
AU - Léveillé, Richard J.
AU - Papineau, Dominic
AU - Rempfert, Kaitlin R.
AU - Sánchez-Román, Mónica
AU - Spear, John R.
AU - Southam, Gordon
AU - Stern, Jennifer C.
AU - Cleaves, Henderson James
N1 - Funding Information:
This article is an outgrowth of an international workshop sponsored by ELSI (Earth-Life Science Institute) EON (ELSI Origins Network) held at the Tokyo Institute of Technology, Japan. The EON is supported by a grant from the John Templeton Foundation. The opinions expressed in this publication are those of the authors and do not necessarily reflect the views of the John Templeton Foundation. The authors thank the group of participants in the workshop who contributed to the development of the ideas and concepts presented here. In addition to the listed authors, they gratefully acknowledge the workshop participation of N. Aubert-Kato, A. Baccouche, N. Bapat, Y. Fuji, C. Giri, S. Ida, J. Kirschvink, I. Mamajanov, A. Panikar, M. Sharma, Y. Ueno, S. Zang, and M. Voytek. The authors gratefully acknowledge two anonymous reviewers who provided helpful comments and suggestions to improve this article.
Publisher Copyright:
© Marjorie A. Chan et al., 2019; Published by Mary Ann Liebert, Inc. 2019.
PY - 2019/9/1
Y1 - 2019/9/1
N2 - 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.
AB - 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.
KW - Astrobiology
KW - Biosignatures
KW - Extraterrestrial life
KW - Extremophile.
KW - Taphonomy
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U2 - 10.1089/ast.2018.1903
DO - 10.1089/ast.2018.1903
M3 - Article
C2 - 31335163
AN - SCOPUS:85066503725
SN - 1531-1074
VL - 19
SP - 1075
EP - 1102
JO - Astrobiology
JF - Astrobiology
IS - 9
ER -