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Final Published Version
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Univ Arizona, Dept AnthropolUniv Arizona, Dept Geosci
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2016-07-08
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Public Library of ScienceCitation
A Blind Test of the Younger Dryas Impact Hypothesis 2016, 11 (7):e0155470 PLOS ONEJournal
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© 2016 Holliday et al. This is an open access article distributed under the terms of the Creative Commons Attribution License.Collection Information
This item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.Abstract
The Younger Dryas Impact Hypothesis (YDIH) states that North America was devastated by some sort of extraterrestrial event similar to 12,800 calendar years before present. Two fundamental questions persist in the debate over the YDIH: Can the results of analyses for purported impact indicators be reproduced? And are the indicators unique to the lower YD boundary (YDB), i.e., similar to 12.8k cal yrs BP? A test reported here presents the results of analyses that address these questions. Two different labs analyzed identical splits of samples collected at, above, and below the similar to 12.8ka zone at the Lubbock Lake archaeological site (LL) in northwest Texas. Both labs reported similar variation in levels of magnetic micrograins (>300 mg/kg >12.8ka and <11.5ka, but <150 mg/kg 12.8ka to 11.5ka). Analysis for magnetic microspheres in one split, reported elsewhere, produced very low to nonexistent levels throughout the section. In the other split, reported here, the levels of magnetic microspherules and nanodiamonds are low or nonexistent at, below, and above the YDB with the notable exception of a sample <11,500 cal years old. In that sample the claimed impact proxies were recovered at abundances two to four orders of magnitude above that from the other samples. Reproducibility of at least some analyses are problematic. In particular, no standard criteria exist for identification of magnetic spheres. Moreover, the purported impact proxies are not unique to the YDB.Note
Open Access JournalISSN
1932-6203Version
Final published versionSponsors
Argonaut Archaeological Research Fund University of Arizona; College of Arts and Sciences, University of WyomingAdditional Links
http://dx.plos.org/10.1371/journal.pone.0155470ae974a485f413a2113503eed53cd6c53
10.1371/journal.pone.0155470
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Except where otherwise noted, this item's license is described as © 2016 Holliday et al. This is an open access article distributed under the terms of the Creative Commons Attribution License.

