A Blind Test of the Younger Dryas Impact Hypothesis

Persistent Link:
http://hdl.handle.net/10150/618977
Title:
A Blind Test of the Younger Dryas Impact Hypothesis
Author:
Holliday, Vance; Surovell, Todd; Johnson, Eileen
Affiliation:
Univ Arizona, Dept Anthropol; Univ Arizona, Dept Geosci
Issue Date:
2016-07-08
Publisher:
Public Library of Science
Citation:
A Blind Test of the Younger Dryas Impact Hypothesis 2016, 11 (7):e0155470 PLOS ONE
Journal:
PLOS ONE
Rights:
© 2016 Holliday et al. This is an open access article distributed under the terms of the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original author and source are credited.
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 Journal
ISSN:
1932-6203
DOI:
10.1371/journal.pone.0155470
Version:
Final published version
Sponsors:
Argonaut Archaeological Research Fund University of Arizona; College of Arts and Sciences, University of Wyoming
Additional Links:
http://dx.plos.org/10.1371/journal.pone.0155470

Full metadata record

DC FieldValue Language
dc.contributor.authorHolliday, Vanceen
dc.contributor.authorSurovell, Todden
dc.contributor.authorJohnson, Eileenen
dc.date.accessioned2016-08-27T00:50:26Z-
dc.date.available2016-08-27T00:50:26Z-
dc.date.issued2016-07-08-
dc.identifier.citationA Blind Test of the Younger Dryas Impact Hypothesis 2016, 11 (7):e0155470 PLOS ONEen
dc.identifier.issn1932-6203-
dc.identifier.doi10.1371/journal.pone.0155470-
dc.identifier.urihttp://hdl.handle.net/10150/618977-
dc.description.abstractThe 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.en
dc.description.sponsorshipArgonaut Archaeological Research Fund University of Arizona; College of Arts and Sciences, University of Wyomingen
dc.language.isoenen
dc.publisherPublic Library of Scienceen
dc.relation.urlhttp://dx.plos.org/10.1371/journal.pone.0155470en
dc.rights© 2016 Holliday et al. This is an open access article distributed under the terms of the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original author and source are credited.en
dc.titleA Blind Test of the Younger Dryas Impact Hypothesisen
dc.typeArticleen
dc.contributor.departmentUniv Arizona, Dept Anthropolen
dc.contributor.departmentUniv Arizona, Dept Geoscien
dc.identifier.journalPLOS ONEen
dc.description.noteOpen Access Journalen
dc.description.collectioninformationThis 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.en
dc.eprint.versionFinal published versionen
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