10
views
0
recommends
+1 Recommend
0 collections
    0
    shares
      • Record: found
      • Abstract: found
      • Article: found
      Is Open Access

      Oxygenation, Life, and the Planetary System during Earth's Middle History: An Overview

      research-article

      Read this article at

      Bookmark
          There is no author summary for this article yet. Authors can add summaries to their articles on ScienceOpen to make them more accessible to a non-specialist audience.

          Abstract

          The long history of life on Earth has unfolded as a cause-and-effect relationship with the evolving amount of oxygen (O 2) in the oceans and atmosphere. Oxygen deficiency characterized our planet's first 2 billion years, yet evidence for biological O 2 production and local enrichments in the surface ocean appear long before the first accumulations of O 2 in the atmosphere roughly 2.4 to 2.3 billion years ago. Much has been written about this fundamental transition and the related balance between biological O 2 production and sinks coupled to deep Earth processes that could buffer against the accumulation of biogenic O 2. However, the relationship between complex life (eukaryotes, including animals) and later oxygenation is less clear. Some data suggest O 2 was higher but still mostly low for another billion and a half years before increasing again around 800 million years ago, potentially setting a challenging course for complex life during its initial development and ecological expansion. The apparent rise in O 2 around 800 million years ago is coincident with major developments in complex life. Multiple geochemical and paleontological records point to a major biogeochemical transition at that time, but whether rising and still dynamic biospheric oxygen triggered or merely followed from innovations in eukaryotic ecology, including the emergence of animals, is still debated. This paper focuses on the geochemical records of Earth's middle history, roughly 1.8 to 0.5 billion years ago, as a backdrop for exploring possible cause-and-effect relationships with biological evolution and the primary controls that may have set its pace, including solid Earth/tectonic processes, nutrient limitation, and their possible linkages. A richer mechanistic understanding of the interplay between coevolving life and Earth surface environments can provide a template for understanding and remotely searching for sustained habitability and even life on distant exoplanets.

          Related collections

          Most cited references202

          • Record: found
          • Abstract: found
          • Article: not found

          The Cambrian conundrum: early divergence and later ecological success in the early history of animals.

          Diverse bilaterian clades emerged apparently within a few million years during the early Cambrian, and various environmental, developmental, and ecological causes have been proposed to explain this abrupt appearance. A compilation of the patterns of fossil and molecular diversification, comparative developmental data, and information on ecological feeding strategies indicate that the major animal clades diverged many tens of millions of years before their first appearance in the fossil record, demonstrating a macroevolutionary lag between the establishment of their developmental toolkits during the Cryogenian [(850 to 635 million years ago (Ma)], and the later ecological success of metazoans during the Ediacaran (635 to 541 Ma) and Cambrian (541 to 488 Ma) periods. We argue that this diversification involved new forms of developmental regulation, as well as innovations in networks of ecological interaction within the context of permissive environmental circumstances.
            Bookmark
            • Record: found
            • Abstract: found
            • Article: not found

            A molecular view of microbial diversity and the biosphere.

            N Pace (1997)
            Over three decades of molecular-phylogenetic studies, researchers have compiled an increasingly robust map of evolutionary diversification showing that the main diversity of life is microbial, distributed among three primary relatedness groups or domains: Archaea, Bacteria, and Eucarya. The general properties of representatives of the three domains indicate that the earliest life was based on inorganic nutrition and that photosynthesis and use of organic compounds for carbon and energy metabolism came comparatively later. The application of molecular-phylogenetic methods to study natural microbial ecosystems without the traditional requirement for cultivation has resulted in the discovery of many unexpected evolutionary lineages; members of some of these lineages are only distantly related to known organisms but are sufficiently abundant that they are likely to have impact on the chemistry of the biosphere.
              Bookmark
              • Record: found
              • Abstract: found
              • Article: not found

              A neoproterozoic snowball earth

              Negative carbon isotope anomalies in carbonate rocks bracketing Neoproterozoic glacial deposits in Namibia, combined with estimates of thermal subsidence history, suggest that biological productivity in the surface ocean collapsed for millions of years. This collapse can be explained by a global glaciation (that is, a snowball Earth), which ended abruptly when subaerial volcanic outgassing raised atmospheric carbon dioxide to about 350 times the modern level. The rapid termination would have resulted in a warming of the snowball Earth to extreme greenhouse conditions. The transfer of atmospheric carbon dioxide to the ocean would result in the rapid precipitation of calcium carbonate in warm surface waters, producing the cap carbonate rocks observed globally.
                Bookmark

                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
                August 2021
                16 August 2021
                16 August 2021
                : 21
                : 8
                : 906-923
                Affiliations
                [ 1 ]Department of Earth and Planetary Sciences, University of California, Riverside, California, USA.
                [ 2 ]Department of Earth and Planetary Sciences, Yale University, New Haven, Connecticut, USA.
                [ 3 ]School of Earth and Atmospheric Sciences, Georgia Institute of Technology, Atlanta, Georgia, USA.
                [ 4 ]State Key Laboratory of Biogeology and Environmental Geology, China University of Geosciences, Wuhan, China.
                Author notes
                [*]Address correspondence to: Timothy W. Lyons, Department of Earth and Planetary Sciences, University of California, Riverside, CA 92521, USA timothy.lyons@ 123456ucr.edu
                Article
                10.1089/ast.2020.2418
                10.1089/ast.2020.2418
                8403206
                34314605
                4916fab2-0131-468a-9dd8-331802d410dc
                © Timothy W. Lyons et al., 2021; 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
                : Submitted 15 December 2020
                : Accepted 25 May 2021
                Page count
                Figures: 3, References: 207, Pages: 18
                Categories
                Special Collection Articles

                biogeochemistry,early earth,coevolving life and environments,oxygen,planetary systems,complex life

                Comments

                Comment on this article