Show simple item record

dc.contributor.authorOsinski, Gordon R.
dc.contributor.authorSpray, John G.
dc.contributor.authorLee, Pascal
dc.date.accessioned2021-02-12T21:18:01Z
dc.date.available2021-02-12T21:18:01Z
dc.date.issued2005-01-01
dc.identifier.citationOsinski, G. R., Spray, J. G., & Lee, P. (2005). Impactites of the Haughton impact structure, Devon island, Canadian High Arctic. Meteoritics & Planetary Science, 40(12), 1789-1812.
dc.identifier.issn1945-5100
dc.identifier.doi10.1111/j.1945-5100.2005.tb00147.x
dc.identifier.urihttp://hdl.handle.net/10150/656077
dc.description.abstractContrary to the previous interpretation of a single allochthonous impactite lithology, combined field, optical, and analytical scanning electron microscopy (SEM) studies have revealed the presence of a series of impactites at the Haughton impact structure. In the crater interior, there is a consistent upward sequence from parautochthonous target rocks overlain by parautochthonous lithic (monomict) breccias, through allochthonous lithic (polymict) breccia, into pale grey allochthonous impact melt breccias. The groundmass of the pale grey impact melt breccias consists of microcrystalline calcite, silicate impact melt glass, and anhydrite. Analytical data and microtextures indicate that these phases represent a series of impact-generated melts that were molten at the time of, and following, deposition. Impact melt glass clasts are present in approximately half of the samples studied. Consideration of the groundmass phases and impact glass clasts reveal that impactites of the crater interior contain shock-melted sedimentary material from depths of >920 to <1880 m in the pre-impact target sequence. Two principal impactites have been recognized in the near-surface crater rim region of Haughton. Pale yellow-brown allochthonous impact melt breccias and megablocks are overlain by pale grey allochthonous impact melt breccias. The former are derived from depths of >200 to <760 m and are interpreted as remnants of the continuous ejecta blanket. The pale grey impact melt breccias, although similar to the impact melt breccias of the crater interior, are more carbonate-rich and do not appear to have incorporated clasts from the crystalline basement. Thus, the spatial distribution of the crater-fill impactites at Haughton, the stratigraphic succession from target rocks to allochthonous impactites, the recognition of large volumes of impact melt breccias, and their probable original volume are all analogous to characteristics of coherent impact melt layers in comparatively sized structures formed in crystalline targets.
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.subjectImpact melt breccias
dc.subjectCarbonate melts
dc.subjectHaughton impact structure
dc.subjectimpactites
dc.subjectCrystalline versus sedimentary targets
dc.titleImpactites of the Haughton impact structure, Devon Island, Canadian High Arctic
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.volume40
dc.source.issue12
dc.source.beginpage1789
dc.source.endpage1812
refterms.dateFOA2021-02-12T21:18:01Z


Files in this item

Thumbnail
Name:
15210-17563-1-PB.pdf
Size:
1.451Mb
Format:
PDF

This item appears in the following Collection(s)

Show simple item record