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dc.contributor.authorKirsimäe, Kalle
dc.contributor.authorSuuroja, Sten
dc.contributor.authorKirs, Juho
dc.contributor.authorKärki, Aulis
dc.contributor.authorPolikarpus, Maile
dc.contributor.authorPuura, Väino
dc.contributor.authorSuuroja, Kalle
dc.date.accessioned2021-02-12T20:55:28Z
dc.date.available2021-02-12T20:55:28Z
dc.date.issued2002-01-01
dc.identifier.citationKirsimäe, K., Suuroja, S., Kirs, J., Kärki, A., Polikarpus, M., Puura, V., & Suuroja, K. (2002). Hornblende alteration and fluid inclusions in Kärdla impact crater, Estonia: Evidence for impact‐induced hydrothermal activity. Meteoritics & Planetary Science, 37(3), 449-457.
dc.identifier.issn1945-5100
dc.identifier.doi10.1111/j.1945-5100.2002.tb00827.x
dc.identifier.urihttp://hdl.handle.net/10150/655490
dc.description.abstractThe well-preserved Kärdla impact crater, on Hiiumaa Island, Estonia, is a 4-km diameter structure formed in a shallow Ordovician sea about 455 Ma ago into a target composed of thin (~150 m) unconsolidated sedimentary layer above a crystalline basement composed of migmatite granites, amphibolites and gneisses. The fractured and crushed amphibolites in the crater area are strongly altered and replaced with secondary chloritic minerals. The most intensive chloritization is found in permeable breccias and heavily shattered basement around and above the central uplift. Alteration is believed to have resulted from convective flow of hydrothermal fluids through the central areas of the crater. Chloritic mineral associations suggest formation temperatures of 100-300 degrees C, in agreement with the most frequent quartz fluid inclusion homogenization temperatures of 150-300 degrees C in allochthonous breccia. The rather low salinity of fluids in Kärdla crater (<13 wt% NaCleq) suggests that the hydrothermal system was recharged either by infiltration of meteoric waters from the cater rim walls raised above sea level after the impact, or by invasion of sea water through the disturbed sedimentary cover and fractured crystalline basement. The well developed hydrothermal system in Kärdla crater shows that the thermal history of the shock heated and uplifted rocks in the central crater area, rather than cooling of impact-melt or suevite sheets, controlled the distribution and intensity of the impact-induced hydrothermal processes.
dc.language.isoen
dc.publisherThe Meteoritical Society
dc.relation.urlhttps://meteoritical.org/
dc.rightsCopyright © The Meteoritical Society
dc.rights.urihttp://rightsstatements.org/vocab/InC/1.0/
dc.subjectHornblende alteration
dc.subjectfluid inclusions
dc.subjectKardla
dc.subjectimpact craters
dc.subjectEstonia
dc.subjecthydrothermal
dc.subjectimpact induced
dc.titleHornblende alteration and fluid inclusions in Kärdla impact crater, Estonia: Evidence for impact-induced hydrothermal activity
dc.typeArticle
dc.typetext
dc.identifier.journalMeteoritics & Planetary Science
dc.description.collectioninformationThe Meteoritics & Planetary Science archives are made available by the Meteoritical Society and the University of Arizona Libraries. Contact lbry-journals@email.arizona.edu for further information.
dc.eprint.versionFinal published version
dc.description.admin-noteMigrated from OJS platform February 2021
dc.source.volume37
dc.source.issue3
dc.source.beginpage449
dc.source.endpage457
refterms.dateFOA2021-02-12T20:55:28Z


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