Halogens in serpentinites from the Isua supracrustal belt, Greenland: An Eoarchean seawater signature and biomass proxy?

dc.contributor.authorDucommun-dit-Verron, Joëlle
dc.contributor.authorKendrick, Mark
dc.contributor.authorBennett, Vickie
dc.contributor.authorNutman, Allen P.
dc.date.accessioned2021-06-23T00:18:50Z
dc.date.issued2019
dc.description.abstractSerpentine in modern seafloor and ophiolitic environments incorporates and often retains high concentrations of atmospheric noble gases and seawater-derived halogens. Ancient serpentinites therefore provide the potential to trace the composition of early surface environments. Antigorite-serpentinites locally carbonated to talc-magnesite schist outcropping in a low strain zone within the Eoarchean Isua supracrustal belt (Greenland) are investigated here, to test the retention of paleo-atmospheric noble gases and Eoarchean seawater halogens, and to further determine the genetic setting and metamorphic history of some of Earth’s oldest serpentinites. Based on field relationships, whole rock major and trace element geochemistry, and mineral chemistry, the investigated serpentinites are shown to represent hydrated and variously carbonated magmatic olivine ± orthopyroxene + Cr-spinel cumulates emplaced at the base of a lava flow of boninitic affinity pillowed in its upper portion. In addition, rare zircons extracted from one of the serpentinised cumulates have distinct magmatic trace element signatures and a U-Pb age of 3721 ± 27 Ma indicating the pillowed lava flow erupted on the Eoarchean seafloor. The serpentinites have high concentrations of noble gases, but the presence of parentless radiogenic ‘excess’ 40Ar, introduced by crustal-derived metamorphic fluids, obscures the 40Ar/36Ar ratio of Eoarchean seawater. Local carbonation of the serpentinites also caused halogen loss and fractionation. However, the least carbonated antigorite serpentinites preserve Br/Cl and I/Cl ratios within the range of modern seafloor serpentinites, which is interpreted as indicating Archaean serpentinising fluids were similar in composition to modern seawater-derived fluids. Importantly, the lowest measured I/Cl ratio of 29 (±2) × 10−6, taken as a maximum value for the Eoarchean ocean, is an order of magnitude lower than estimates for the primitive mantle I/Cl value. Iodine has a low concentration relative to Cl in modern seawater because it is sequestered by organic matter. If the inferred low I/Cl of Eoarchean seawater is correct, then similar I-sequestration was likely occurring in the Eoarchean, a process requiring the presence of significant biomass in Earth’s early oceans. Further constraining the Precambrian evolution of seawater I/Cl via serpentinites or other proxies may provide a novel method to explore the emergence and evolution of terrestrial biomass.en_AU
dc.description.sponsorshipMark Kendrick was supported by an Australian Research Council Future Fellowship (no. FT130100141). Support for this work was provided by ARC Discovery Projects DP120102225 and DP170100715.en_AU
dc.identifier.issn0016-7037en_AU
dc.identifier.urihttp://hdl.handle.net/1885/237904
dc.publisherPergamon Press Ltd.en_AU
dc.relationhttp://purl.org/au-research/grants/arc/FT130100141en_AU
dc.relationhttp://purl.org/au-research/grants/arc/DP120102225en_AU
dc.relationhttp://purl.org/au-research/grants/arc/DP170100715en_AU
dc.rights© 2019 Crown Copyrighten_AU
dc.sourceGeochimica et Cosmochimica Actaen_AU
dc.subjectEarly earthen_AU
dc.subjectHalogensen_AU
dc.subjectSerpentinitesen_AU
dc.subjectEarly lifeen_AU
dc.subjectIsua supracrustal belt (ISB)en_AU
dc.titleHalogens in serpentinites from the Isua supracrustal belt, Greenland: An Eoarchean seawater signature and biomass proxy?en_AU
dc.typeJournal articleen_AU
dcterms.dateAccepted2019-07-05
local.bibliographicCitation.lastpage59en_AU
local.bibliographicCitation.startpage31en_AU
local.contributor.affiliationDucommun-dit-Verron, Joëlle, College of Science, ANUen_AU
local.contributor.affiliationKendrick, Mark, College of Science, ANUen_AU
local.contributor.affiliationBennett, Vickie, College of Science, ANUen_AU
local.contributor.affiliationNutman, Allen P., University of Wollongongen_AU
local.contributor.authoruidDucommun-dit-Verron, Joëlle, u5679218en_AU
local.contributor.authoruidKendrick, Mark, u4746994en_AU
local.contributor.authoruidBennett, Vickie, u8904005en_AU
local.description.embargo2099-12-31
local.description.notesAdded manually as didn't import from ARIESen_AU
local.identifier.absfor040203 - Isotope Geochemistryen_AU
local.identifier.absfor040303 - Geochronologyen_AU
local.identifier.absfor040304 - Igneous and Metamorphic Petrologyen_AU
local.identifier.absseo970104 - Expanding Knowledge in the Earth Sciencesen_AU
local.identifier.ariespublicationu3102795xPUB4507en_AU
local.identifier.citationvolume262en_AU
local.identifier.doi10.1016/j.gca.2019.07.017en_AU
local.publisher.urlhttps://www.sciencedirect.com/en_AU
local.type.statusPublished Versionen_AU

Downloads

Original bundle

Now showing 1 - 1 of 1
Loading...
Thumbnail Image
Name:
1-s2.0-S0016703719304272-main.pdf
Size:
5.45 MB
Format:
Adobe Portable Document Format
Description: