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dc.contributor.authorHecht, L.
dc.contributor.authorReimold, W. U.
dc.contributor.authorSherlock, S.
dc.contributor.authorTagle, R.
dc.contributor.authorKoeberl, C.
dc.contributor.authorSchmitt, R.-T.
dc.date.accessioned2021-02-12T22:30:59Z
dc.date.available2021-02-12T22:30:59Z
dc.date.issued2008-01-01
dc.identifier.citationHecht, L., Reimold, W. U., Sherlock, S., Tagle, R., Koeberl, C., & Schmitt, R.-T. (2008). New impact‐melt rock from the Roter Kamm impact structure, Namibia: Further constraints on impact age, melt rock chemistry, and projectile composition. Meteoritics & Planetary Science, 43(7), 1201-1218.
dc.identifier.issn1945-5100
dc.identifier.doi10.1111/j.1945-5100.2008.tb01123.x
dc.identifier.urihttp://hdl.handle.net/10150/656455
dc.description.abstractA new locality of in situ massive impact-melt rock was discovered on the southsouthwestern rim of the Roter Kamm impact structure. While the sub-samples from this new locality are relatively homogeneous at the hand specimen scale, and despite being from a nearby location, they do not have the same composition of the only previously analyzed impact-melt rock sample from Roter Kamm. Both Roter Kamm impact-melt rock samples analyzed to date, as well as several suevite samples, exhibit a granitic-granodioritic precursor composition. Micro-chemical analyses of glassy matrix and Al-rich orthopyroxene microphenocrysts demonstrate rapid cooling and chemical disequilibrium at small scales. Platinum-group element abundances and ratios indicate an ordinary chondritic composition for the Roter Kamm impactor. Laser argon dating of two sub-samples did not reproduce the previously obtained age of 3.7 +/- 0.3 (1-sigma) for this impact event, based on 40Ar/39Ar dating of a single vesicular impact-melt rock. Instead, we obtained ages between 3.9 and 6.3 Ma, with an inverse isochron age of 4.7 +/- 0.3 Ma for one analyzed sub-sample and 5.1 +/- 0.4 Ma for the other. Clearly a post-5 Ma impact at Roter Kamm remains indicated, but further analytical work is required to better constrain the currently best estimate of 4-5 Ma. Both impactor and age constraints are clearly obstructed by the inherent microscopic heterogeneity and disequilibrium melting and cooling processes demonstrated in the present study.
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.subjectRoter Kamm
dc.subjectNamibia Impact crater
dc.subjectDating
dc.subjectgeochemistry
dc.subjectmelts
dc.titleNew impact-melt rock from the Roter Kamm impact structure, Namibia: Further constraints on impact age, melt rock chemistry, and projectile composition
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.volume43
dc.source.issue7
dc.source.beginpage1201
dc.source.endpage1218
refterms.dateFOA2021-02-12T22:30:59Z


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