Show simple item record

dc.contributor.authorDeutsch, Alexander
dc.contributor.authorKoeberl, Christian
dc.date.accessioned2021-02-12T21:40:34Z
dc.date.available2021-02-12T21:40:34Z
dc.date.issued2006-01-01
dc.identifier.citationDeutsch, A., & Koeberl, C. (2006). Establishing the link between the Chesapeake Bay impact structure and the North American tektite strewn field: The Sr‐Nd isotopic evidence. Meteoritics & Planetary Science, 41(5), 689-703.
dc.identifier.issn1945-5100
dc.identifier.doi10.1111/j.1945-5100.2006.tb00985.x
dc.identifier.urihttp://hdl.handle.net/10150/656131
dc.description.abstractThe Chesapeake Bay impact structure, which is about 35 Ma old, has previously been proposed as the possible source crater of the North American tektites (NAT). Here we report major and trace element data as well as the first Sr-Nd isotope data for drill core and outcrop samples of target lithologies, crater fill breccias, and post-impact sediments of the Chesapeake Bay impact structure. The unconsolidated sediments, Cretaceous to middle Eocene in age, have epsilon-Srt = 35.7 Ma of +54 to +272, and epsilon-Ndt = 35.7 Ma ranging from -6.5 to -10.8; one sample from the granitic basement with a TNdCHUR model age of 1.36 Ga yielded an epsilon-Srt = 35.7 Ma of +188 and an epsilon-Ndt = 35.7 Ma of -5.7. The Exmore breccia (crater fill) can be explained as a mix of the measured target sediments and the granite, plus an as-yet undetermined component. The post-impact sediments of the Chickahominy formation have slightly higher TNdCHUR model ages of about 1.55 Ga, indicating a contribution of some older materials. Newly analyzed bediasites have the following isotope parameters: +104 to +119 (epsilon-Srt = 35.7 Ma), -5.7 (epsilon-Ndt = 35.7 Ma), 0.47 Ga (TSrUR), and 1.15 Ga (TNdCHUR), which is in excellent agreement with previously published data for samples of the NAT strewn field. Target rocks with highly radiogenic Sr isotopic composition, as required for explaining the isotopic characteristics of Deep Sea Drilling Project (DSDP) site 612 tektites, were not among the analyzed sample suite. Based on the new isotope data, we exclude any relation between the NA tektites and the Popigai impact crater, although they have identical ages within 2 errors. The Chesapeake Bay structure, however, is now clearly constrained as the source crater for the North American tektites, although the present data set obviously does not include all target lithologies that have contributed to the composition of the tektites.
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.subjectVirginia
dc.subjectimpact crater USA
dc.subjectisotope geochemistry
dc.subjectChesapeake Bay
dc.subjectTektites
dc.subjecttrace elements
dc.titleEstablishing the link between the Chesapeake Bay impact structure and the North American tektite strewn field: The Sr-Nd isotopic evidence
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.volume41
dc.source.issue5
dc.source.beginpage689
dc.source.endpage703
refterms.dateFOA2021-02-12T21:40:34Z


Files in this item

Thumbnail
Name:
15270-17623-1-PB.pdf
Size:
2.381Mb
Format:
PDF

This item appears in the following Collection(s)

Show simple item record