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Temporal variation of planetary iron as a driver of evolution.

Λεπτομέρειες βιβλιογραφικής εγγραφής
Τίτλος: Temporal variation of planetary iron as a driver of evolution.
Συγγραφείς: Wade J; Department of Earth Sciences, University of Oxford, Oxford OX1 3AN, United Kingdom; jon.wade@earth.ox.ac.uk chris.ballentine@earth.ox.ac.uk alexander.drakesmith@imm.ox.ac.uk., Byrne DJ; Centre de Recherches Pétrographiques et Géochimiques, UMR 7358 CNRS-Université de Lorraine, BP 20, F-54501 Vandoeuvre-lés-Nancy, France., Ballentine CJ; Department of Earth Sciences, University of Oxford, Oxford OX1 3AN, United Kingdom; jon.wade@earth.ox.ac.uk chris.ballentine@earth.ox.ac.uk alexander.drakesmith@imm.ox.ac.uk., Drakesmith H; MRC (Medical Research Council) Human Immunology Unit, MRC Weatherall Institute of Molecular Medicine, Radcliffe Department of Medicine, University of Oxford, Oxford OX3 9DS, United Kingdom jon.wade@earth.ox.ac.uk chris.ballentine@earth.ox.ac.uk alexander.drakesmith@imm.ox.ac.uk.
Πηγή: Proceedings of the National Academy of Sciences of the United States of America [Proc Natl Acad Sci U S A] 2021 Dec 21; Vol. 118 (51).
Τύπος έκδοσης: Journal Article; Research Support, Non-U.S. Gov't
Γλώσσα: English
Στοιχεία περιοδικού: Publisher: National Academy of Sciences Country of Publication: United States NLM ID: 7505876 Publication Model: Print Cited Medium: Internet ISSN: 1091-6490 (Electronic) Linking ISSN: 00278424 NLM ISO Abbreviation: Proc Natl Acad Sci U S A Subsets: MEDLINE
Imprint Name(s): Original Publication: Washington, DC : National Academy of Sciences
Ιατρικοί όροι (MeSH): Biological Evolution* , Evolution, Planetary*, Iron/*metabolism, Iron/chemistry ; Siderophores/metabolism ; Water/chemistry ; Water/metabolism ; Biological Availability ; Earth, Planet ; Ecosystem ; Genetic Variation ; Geology ; Host-Pathogen Interactions ; Oxidation-Reduction
Περίληψη: Iron is an irreplaceable component of proteins and enzyme systems required for life. This need for iron is a well-characterized evolutionary mechanism for genetic selection. However, there is limited consideration of how iron bioavailability, initially determined by planetary accretion but fluctuating considerably at global scale over geological time frames, has shaped the biosphere. We describe influences of iron on planetary habitability from formation events >4 Gya and initiation of biochemistry from geochemistry through oxygenation of the atmosphere to current host-pathogen dynamics. By determining the iron and transition element distribution within the terrestrial planets, planetary core formation is a constraint on both the crustal composition and the longevity of surface water, hence a planet's habitability. As such, stellar compositions, combined with metallic core-mass fraction, may be an observable characteristic of exoplanets that relates to their ability to support life. On Earth, the stepwise rise of atmospheric oxygen effectively removed gigatons of soluble ferrous iron from habitats, generating evolutionary pressures. Phagocytic, infectious, and symbiotic behaviors, dating from around the Great Oxygenation Event, refocused iron acquisition onto biotic sources, while eukaryotic multicellularity allows iron recycling within an organism. These developments allow life to more efficiently utilize a scarce but vital nutrient. Initiation of terrestrial life benefitted from the biochemical properties of abundant mantle/crustal iron, but the subsequent loss of iron bioavailability may have been an equally important driver of compensatory diversity. This latter concept may have relevance for the predicted future increase in iron deficiency across the food chain caused by elevated atmospheric CO2.
(Copyright © 2021 the Author(s). Published by PNAS.)
Competing Interests: The authors declare no competing interest.
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Grant Information: MC_UU_00008/10 United Kingdom MRC_ Medical Research Council; MC_UU_12010/10 United Kingdom MRC_ Medical Research Council
Contributed Indexing: Keywords: complex life; evolution; iron; oxygenation; planetary habitability
Substance Nomenclature: 0 (Siderophores)
059QF0KO0R (Water)
E1UOL152H7 (Iron)
Entry Date(s): Date Created: 20211207 Date Completed: 20220113 Latest Revision: 20250530
Update Code: 20260130
PubMed Central ID: PMC8713747
DOI: 10.1073/pnas.2109865118
PMID: 34873026
Βάση Δεδομένων: MEDLINE
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  Data: Temporal variation of planetary iron as a driver of evolution.
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  Data: <searchLink fieldCode="AU" term="%22Wade+J%22">Wade J</searchLink>; Department of Earth Sciences, University of Oxford, Oxford OX1 3AN, United Kingdom; jon.wade@earth.ox.ac.uk chris.ballentine@earth.ox.ac.uk alexander.drakesmith@imm.ox.ac.uk.<br /><searchLink fieldCode="AU" term="%22Byrne+DJ%22">Byrne DJ</searchLink>; Centre de Recherches Pétrographiques et Géochimiques, UMR 7358 CNRS-Université de Lorraine, BP 20, F-54501 Vandoeuvre-lés-Nancy, France.<br /><searchLink fieldCode="AU" term="%22Ballentine+CJ%22">Ballentine CJ</searchLink>; Department of Earth Sciences, University of Oxford, Oxford OX1 3AN, United Kingdom; jon.wade@earth.ox.ac.uk chris.ballentine@earth.ox.ac.uk alexander.drakesmith@imm.ox.ac.uk.<br /><searchLink fieldCode="AU" term="%22Drakesmith+H%22">Drakesmith H</searchLink>; MRC (Medical Research Council) Human Immunology Unit, MRC Weatherall Institute of Molecular Medicine, Radcliffe Department of Medicine, University of Oxford, Oxford OX3 9DS, United Kingdom jon.wade@earth.ox.ac.uk chris.ballentine@earth.ox.ac.uk alexander.drakesmith@imm.ox.ac.uk.
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  Data: <searchLink fieldCode="JN" term="%227505876%22">Proceedings of the National Academy of Sciences of the United States of America</searchLink> [Proc Natl Acad Sci U S A] 2021 Dec 21; Vol. 118 (51).
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  Data: <searchLink fieldCode="MM" term="%22Biological+Evolution%22">Biological Evolution*</searchLink> <br /><searchLink fieldCode="MM" term="%22Evolution%2C+Planetary%22">Evolution, Planetary*</searchLink><br /><searchLink fieldCode="MM" term="%22Iron%22">Iron</searchLink>/<searchLink fieldCode="MM" term="%22Iron+metabolism%22">*metabolism</searchLink><br /><searchLink fieldCode="MH" term="%22Iron%22">Iron</searchLink>/<searchLink fieldCode="MH" term="%22Iron+chemistry%22">chemistry</searchLink> ; <searchLink fieldCode="MH" term="%22Siderophores%22">Siderophores</searchLink>/<searchLink fieldCode="MH" term="%22Siderophores+metabolism%22">metabolism</searchLink> ; <searchLink fieldCode="MH" term="%22Water%22">Water</searchLink>/<searchLink fieldCode="MH" term="%22Water+chemistry%22">chemistry</searchLink> ; <searchLink fieldCode="MH" term="%22Water%22">Water</searchLink>/<searchLink fieldCode="MH" term="%22Water+metabolism%22">metabolism</searchLink> ; <searchLink fieldCode="MH" term="%22Biological+Availability%22">Biological Availability</searchLink> ; <searchLink fieldCode="MH" term="%22Earth%2C+Planet%22">Earth, Planet</searchLink> ; <searchLink fieldCode="MH" term="%22Ecosystem%22">Ecosystem</searchLink> ; <searchLink fieldCode="MH" term="%22Genetic+Variation%22">Genetic Variation</searchLink> ; <searchLink fieldCode="MH" term="%22Geology%22">Geology</searchLink> ; <searchLink fieldCode="MH" term="%22Host-Pathogen+Interactions%22">Host-Pathogen Interactions</searchLink> ; <searchLink fieldCode="MH" term="%22Oxidation-Reduction%22">Oxidation-Reduction</searchLink>
– Name: Abstract
  Label: Abstract
  Group: Ab
  Data: Iron is an irreplaceable component of proteins and enzyme systems required for life. This need for iron is a well-characterized evolutionary mechanism for genetic selection. However, there is limited consideration of how iron bioavailability, initially determined by planetary accretion but fluctuating considerably at global scale over geological time frames, has shaped the biosphere. We describe influences of iron on planetary habitability from formation events >4 Gya and initiation of biochemistry from geochemistry through oxygenation of the atmosphere to current host-pathogen dynamics. By determining the iron and transition element distribution within the terrestrial planets, planetary core formation is a constraint on both the crustal composition and the longevity of surface water, hence a planet's habitability. As such, stellar compositions, combined with metallic core-mass fraction, may be an observable characteristic of exoplanets that relates to their ability to support life. On Earth, the stepwise rise of atmospheric oxygen effectively removed gigatons of soluble ferrous iron from habitats, generating evolutionary pressures. Phagocytic, infectious, and symbiotic behaviors, dating from around the Great Oxygenation Event, refocused iron acquisition onto biotic sources, while eukaryotic multicellularity allows iron recycling within an organism. These developments allow life to more efficiently utilize a scarce but vital nutrient. Initiation of terrestrial life benefitted from the biochemical properties of abundant mantle/crustal iron, but the subsequent loss of iron bioavailability may have been an equally important driver of compensatory diversity. This latter concept may have relevance for the predicted future increase in iron deficiency across the food chain caused by elevated atmospheric CO<subscript>2</subscript>.<br /> (Copyright © 2021 the Author(s). Published by PNAS.)
– Name: Abstract
  Label: Competing Interests
  Group: Ab
  Data: The authors declare no competing interest.
– Name: Ref
  Label: References
  Group: RefInfo
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        Text: English
    Subjects:
      – SubjectFull: Iron chemistry
        Type: general
      – SubjectFull: Siderophores metabolism
        Type: general
      – SubjectFull: Water chemistry
        Type: general
      – SubjectFull: Water metabolism
        Type: general
      – SubjectFull: Biological Availability
        Type: general
      – SubjectFull: Earth, Planet
        Type: general
      – SubjectFull: Ecosystem
        Type: general
      – SubjectFull: Genetic Variation
        Type: general
      – SubjectFull: Geology
        Type: general
      – SubjectFull: Host-Pathogen Interactions
        Type: general
      – SubjectFull: Oxidation-Reduction
        Type: general
      – SubjectFull: Biological Evolution
        Type: general
      – SubjectFull: Evolution, Planetary
        Type: general
      – SubjectFull: Iron metabolism
        Type: general
    Titles:
      – TitleFull: Temporal variation of planetary iron as a driver of evolution.
        Type: main
  BibRelationships:
    HasContributorRelationships:
      – PersonEntity:
          Name:
            NameFull: Wade J
      – PersonEntity:
          Name:
            NameFull: Byrne DJ
      – PersonEntity:
          Name:
            NameFull: Ballentine CJ
      – PersonEntity:
          Name:
            NameFull: Drakesmith H
    IsPartOfRelationships:
      – BibEntity:
          Dates:
            – D: 21
              M: 12
              Text: 2021 Dec 21
              Type: published
              Y: 2021
          Identifiers:
            – Type: issn-electronic
              Value: 1091-6490
          Numbering:
            – Type: volume
              Value: 118
            – Type: issue
              Value: 51
          Titles:
            – TitleFull: Proceedings of the National Academy of Sciences of the United States of America
              Type: main
ResultId 1