Please use this identifier to cite or link to this item: https://hdl.handle.net/1959.11/63113
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dc.contributor.authorTrail, Dustinen
dc.contributor.authorTailby, Nicholas Den
dc.contributor.authorSochko, Maggieen
dc.contributor.authorAckerson, Michael Ren
dc.date.accessioned2024-09-24T00:26:37Z-
dc.date.available2024-09-24T00:26:37Z-
dc.date.issued2015-07-22-
dc.identifier.citationAstrobiology, 15(7), p. 575-586en
dc.identifier.issn1557-8070en
dc.identifier.issn1531-1074en
dc.identifier.urihttps://hdl.handle.net/1959.11/63113-
dc.description.abstract<p>Granitoids are silicic rocks that make up the majority of the continental crust, but different models arise for the origins of these rocks. One classification scheme defines different granitoid types on the basis of materials involved in the melting/crystallization process. In this end-member case, granitoids may be derived from melting of a preexisting igneous rock, while other granitoids, by contrast, are formed or influenced by melting of buried sedimentary material. In the latter case, assimilated sedimentary material altered by chemical processes occurring at the near surface of Earth—including biological activity—could influence magma chemical properties. Here, we apply a redox-sensitive calibration based on the incorporation of Ce into zircon crystals found in these two rock types, termed sedimentary-type (S-type) and igneous-type (I-type) granitoids. The ~400 Ma Lachlan Fold Belt rocks of southeastern Australia were chosen for investigation here; these rocks have been a key target used to describe and explore granitoid genesis for close to 50 years. We observe that zircons found in S-type granitoids formed under more reducing conditions than those formed from I-type granitoids from the same terrain. This observation, while reflecting 9 granitoids and 289 analyses of zircons from a region where over 400 different plutons have been identified, is consistent with the incorporation of (reduced) organic matter in the former and highlights one possible manner in which life may modify the composition of igneous minerals. The chemical properties of rocks or igneous minerals may extend the search for ancient biological activity to the earliest period of known igneous activity, which dates back to ~4.4 billion years ago. If organic matter was incorporated into Hadean sediments that were buried and melted, then these biological remnants could imprint a chemical signature within the subsequent melt and the resulting crystal assemblage, including zircon.</p>en
dc.languageenen
dc.publisherMary Ann Liebert, Inc Publishersen
dc.relation.ispartofAstrobiologyen
dc.titlePossible Biosphere-Lithosphere Interactions Preserved in Igneous Zircon and Implications for Hadean Earthen
dc.typeJournal Articleen
dc.identifier.doi10.1089/ast.2014.1248en
local.contributor.firstnameDustinen
local.contributor.firstnameNicholas Den
local.contributor.firstnameMaggieen
local.contributor.firstnameMichael Ren
local.profile.schoolSchool of Environmental & Rural Scienceen
local.profile.emailntailby@une.edu.auen
local.output.categoryC1en
local.record.placeauen
local.record.institutionUniversity of New Englanden
local.publisher.placeUnited States of Americaen
local.format.startpage575en
local.format.endpage586en
local.peerreviewedYesen
local.identifier.volume15en
local.identifier.issue7en
local.contributor.lastnameTrailen
local.contributor.lastnameTailbyen
local.contributor.lastnameSochkoen
local.contributor.lastnameAckersonen
dc.identifier.staffune-id:ntailbyen
local.profile.orcid0000-0002-2305-3338en
local.profile.roleauthoren
local.profile.roleauthoren
local.profile.roleauthoren
local.profile.roleauthoren
local.identifier.unepublicationidune:1959.11/63113en
local.date.onlineversion2015-07-08-
dc.identifier.academiclevelAcademicen
dc.identifier.academiclevelAcademicen
dc.identifier.academiclevelAcademicen
dc.identifier.academiclevelAcademicen
local.title.maintitlePossible Biosphere-Lithosphere Interactions Preserved in Igneous Zircon and Implications for Hadean Earthen
local.output.categorydescriptionC1 Refereed Article in a Scholarly Journalen
local.search.authorTrail, Dustinen
local.search.authorTailby, Nicholas Den
local.search.authorSochko, Maggieen
local.search.authorAckerson, Michael Ren
local.uneassociationNoen
local.atsiresearchNoen
local.sensitive.culturalNoen
local.year.available2015en
local.year.published2015en
local.subject.for2020370503 Igneous and metamorphic petrologyen
local.subject.for2020370502 Geochronologyen
local.subject.for2020370507 Planetary geologyen
local.codeupdate.date2024-11-01T17:06:54.580en
local.codeupdate.epersonntailby@une.edu.auen
local.codeupdate.finalisedtrueen
local.original.for20203705 Geologyen
local.profile.affiliationtypeExternal Affiliationen
local.profile.affiliationtypeExternal Affiliationen
local.profile.affiliationtypeExternal Affiliationen
local.profile.affiliationtypeExternal Affiliationen
local.date.moved2024-09-24en
Appears in Collections:Journal Article
School of Environmental and Rural Science
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