Geochemistry of 2.63-2.49Ga impact spherule layers and implications for stratigraphic correlations and impact processes

Title:
Geochemistry of 2.63-2.49Ga impact spherule layers and implications for stratigraphic correlations and impact processes
Authors:
Simonson, Bruce M.; McDonald, Iain; Shukolyukov, Alex; Koeberl, Christian; Reimold, Wolf Uwe; Lugmair, Günter W.
Abstract:
Thin layers rich in spherules formed during impacts by large extraterrestrial objects have the potential to shed new light on impact processes and aid in the long-distance stratigraphic correlation of Precambrian successions. Seven formations in Western Australia and South Africa clustered around the Archean-Proterozoic boundary each contain a single spherule layer, all of which were deposited between ca. 2.49 and 2.63Ga. Analyses of 25 samples from 6 of the 7 spherule layers and 23 samples from closely associated strata free of spherules revealed an extraterrestrial component (ETC) in all six layers, based on PGE ratios and/or Cr isotopic composition. The amount of ETC varies from marginally detectable to clear and obvious; it generally amounts to ca. a few percent. Both PGE ratios and Cr isotopic anomalies indicate most if not all of the impactors were ordinary chondritic in composition. In contrast, all spherule layers older than ca. 3.0Ga that have been analyzed were produced by carbonaceous chondritic impactors. Normalized rare earth element patterns suggest most target rocks were basaltic in composition and variability in PGE ratios favors ballistic emplacement of melt droplets rather than spherule formation via vapor condensation. The geochemical data also provide a means to test proposed intra- and intercontinental stratigraphic correlations. Cr isotopic compositions are consistent with the formation of the oldest layers on both continents by a single impact event about 2.63Ga. In contrast, clear geochemical differences between the middle layers, both deposited ca. 2.54Ga, suggest they were not produced by the same impact event. The youngest, banded iron formation-hosted layers on both continents have also been correlated, but no geochemical data are available on the African layer to test this at present.
Citation:
Simonson, B.M., I. McDonald, A. Shukolyukov, C. Koeberl, W.U. Reimold, G.W. Lugmair. 2009. "Geochemistry of 2.63-2.49 Ga impact spherule layers and implications for stratigraphic correlations and impact processes." Precambrian Research 175(1-4): 51-76.
Publisher:
Elsevier
DATE ISSUED:
2009-12
Department:
Geology
Type:
article
PUBLISHED VERSION:
10.1016/j.precamres.2009.08.004
Additional Links:
http://journals.ohiolink.edu/ejc/article.cgi?issn=03019268&issue=v175i1-4&article=51_go2islfscaip
PERMANENT LINK:
http://hdl.handle.net/11282/309435

Full metadata record

DC FieldValue Language
dc.contributor.authorSimonson, Bruce M.en_US
dc.contributor.authorMcDonald, Iainen_US
dc.contributor.authorShukolyukov, Alexen_US
dc.contributor.authorKoeberl, Christianen_US
dc.contributor.authorReimold, Wolf Uween_US
dc.contributor.authorLugmair, Günter W.en_US
dc.date.accessioned2013-12-23T16:09:35Zen
dc.date.available2013-12-23T16:09:35Zen
dc.date.issued2009-12en
dc.identifier.citationSimonson, B.M., I. McDonald, A. Shukolyukov, C. Koeberl, W.U. Reimold, G.W. Lugmair. 2009. "Geochemistry of 2.63-2.49 Ga impact spherule layers and implications for stratigraphic correlations and impact processes." Precambrian Research 175(1-4): 51-76.en_US
dc.identifier.issn0301-9268en_US
dc.identifier.urihttp://hdl.handle.net/11282/309435en
dc.description.abstractThin layers rich in spherules formed during impacts by large extraterrestrial objects have the potential to shed new light on impact processes and aid in the long-distance stratigraphic correlation of Precambrian successions. Seven formations in Western Australia and South Africa clustered around the Archean-Proterozoic boundary each contain a single spherule layer, all of which were deposited between ca. 2.49 and 2.63Ga. Analyses of 25 samples from 6 of the 7 spherule layers and 23 samples from closely associated strata free of spherules revealed an extraterrestrial component (ETC) in all six layers, based on PGE ratios and/or Cr isotopic composition. The amount of ETC varies from marginally detectable to clear and obvious; it generally amounts to ca. a few percent. Both PGE ratios and Cr isotopic anomalies indicate most if not all of the impactors were ordinary chondritic in composition. In contrast, all spherule layers older than ca. 3.0Ga that have been analyzed were produced by carbonaceous chondritic impactors. Normalized rare earth element patterns suggest most target rocks were basaltic in composition and variability in PGE ratios favors ballistic emplacement of melt droplets rather than spherule formation via vapor condensation. The geochemical data also provide a means to test proposed intra- and intercontinental stratigraphic correlations. Cr isotopic compositions are consistent with the formation of the oldest layers on both continents by a single impact event about 2.63Ga. In contrast, clear geochemical differences between the middle layers, both deposited ca. 2.54Ga, suggest they were not produced by the same impact event. The youngest, banded iron formation-hosted layers on both continents have also been correlated, but no geochemical data are available on the African layer to test this at present.en_US
dc.language.isoen_USen_US
dc.publisherElsevieren_US
dc.identifier.doi10.1016/j.precamres.2009.08.004en_US
dc.relation.urlhttp://journals.ohiolink.edu/ejc/article.cgi?issn=03019268&issue=v175i1-4&article=51_go2islfscaipen_GB
dc.subject.departmentGeologyen_US
dc.titleGeochemistry of 2.63-2.49Ga impact spherule layers and implications for stratigraphic correlations and impact processesen_US
dc.typearticleen_US
dc.identifier.journalPrecambrian Researchen_US
dc.subject.keywordSpherulesen_US
dc.subject.keywordImpact ejectaen_US
dc.subject.keywordNeoarcheanen_US
dc.subject.keywordPaleoproterozoicen_US
dc.subject.keywordHamersleyen_US
dc.subject.keywordTransvaalen_US
dc.identifier.volume175en_US
dc.identifier.issue1-4en_US
dc.identifier.startpage51en_US
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