Impact glasses from Belize represent tektites from the Pleistocene Pantasma impact crater in Nicaragua.


Journal

Communications earth & environment
ISSN: 2662-4435
Titre abrégé: Commun Earth Environ
Pays: England
ID NLM: 101772745

Informations de publication

Date de publication:
17 May 2021
Historique:
entrez: 19 8 2021
pubmed: 20 8 2021
medline: 20 8 2021
Statut: ppublish

Résumé

Tektites are terrestrial impact-generated glasses that are ejected long distance (up to 11,000 km), share unique characteristics and have a poorly understood formation process. Only four tektite strewn-fields are known, and three of them are sourced from known impact craters. Here we show that the recently discovered Pantasma impact crater (14 km diameter) in Nicaragua is the source of an impact glass strewn-field documented in Belize 530 km away. Their cogenesis is documented by coincidental ages, at 804 ± 9 ka, as well as consistent elemental compositions and isotopic ratios. The Belize impact glass share many characteristics with known tektites but also present several peculiar features. We propose that these glasses represent a previously unrecognized tektite strewn-field. These discoveries shed new light on the tektite formation process, which may be more common than previously claimed, as most known Pleistocene >10 km diameter cratering events have generated tektites.

Identifiants

pubmed: 34409303
doi: 10.1038/s43247-021-00155-1
pmc: PMC7611520
mid: EMS131201
doi:

Types de publication

Journal Article

Langues

eng

Pagination

94

Subventions

Organisme : European Research Council
ID : 833275
Pays : International

Déclaration de conflit d'intérêts

Competing interests The authors declare no competing interests

Références

Science. 2016 Oct 14;354(6309):225-229
pubmed: 27738171
Astrobiology. 2020 Jan;20(1):91-141
pubmed: 31880475
Proc Natl Acad Sci U S A. 2020 Jan 21;117(3):1346-1353
pubmed: 31889003

Auteurs

Pierre Rochette (P)

Aix-Marseille Université, CNRS, IRD, INRAE, UM 34 CEREGE, Aix-en-Provence, France.

Pierre Beck (P)

IPAG Université Grenoble Alpes, CNRS, Institut de Planétologie et d'Astrophysique de Grenoble, Grenoble, France.

Martin Bizzarro (M)

Centre for Star and Planet Formation, Globe Institute, University of Copenhagen, Copenhagen, Denmark.

Régis Braucher (R)

Aix-Marseille Université, CNRS, IRD, INRAE, UM 34 CEREGE, Aix-en-Provence, France.

Jean Cornec (J)

Geologist, Denver, USA.

Vinciane Debaille (V)

Laboratoire G-Time, Université Libre de Bruxelles, Brussels, Belgium.

Bertrand Devouard (B)

Aix-Marseille Université, CNRS, IRD, INRAE, UM 34 CEREGE, Aix-en-Provence, France.

Jérôme Gattacceca (J)

Aix-Marseille Université, CNRS, IRD, INRAE, UM 34 CEREGE, Aix-en-Provence, France.

Fred Jourdan (F)

School of Earth and Planetary Sciences, Curtin University, Perth, Australia.

Fabien Moustard (F)

Aix-Marseille Université, CNRS, IRD, INRAE, UM 34 CEREGE, Aix-en-Provence, France.

Frédéric Moynier (F)

Institut de Physique du Globe de Paris, Université Sorbonne Paris Cité, CNRS UMR 7154, Paris, France.

Sébastien Nomade (S)

LSCE, CEA, UVSQ et Université Paris-Saclay UMR 8212, Gif-sur-Yvette, France.

Bruno Reynard (B)

Université de Lyon, ENSL, UCBL, CNRS, LGL-TPE, Lyon, France.

Classifications MeSH