Volume 54, Issue 7 p. 1431-1461
Original Article

The CM carbonaceous chondrite regolith Diepenveen

Marco Langbroek,

Department of Research & Education, Naturalis Biodiversity Center, Darwinweg 2, 2333 CR Leiden, the Netherlands

Dutch Meteor Society, Leiden, the Netherlands

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Peter Jenniskens,

Corresponding Author

Dutch Meteor Society, Leiden, the Netherlands

SETI Institute, 189 Bernardo Ave, Mountain View, California, 94043 USA

Corresponding author. E-mail: Petrus.M.Jenniskens@nasa.govSearch for more papers by this author
Leo M. Kriegsman,

Department of Research & Education, Naturalis Biodiversity Center, Darwinweg 2, 2333 CR Leiden, the Netherlands

Department of Earth Sciences, Utrecht University, Princetonlaan 8A, 3584 CB Utrecht, the Netherlands

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Henk Nieuwenhuis,

Koninklijk Eise Eisinga Planetarium, Eisingastraat 3, 8801 KE Franeker, the Netherlands

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Niek De Kort,

Meteor Section, Royal Netherlands Association for Meteorology and Astronomy, Asmansweg 50, 2571 BK Den Haag, the Netherlands

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Jacob Kuiper,

Royal Netherlands Meteorological Institute, Utrechtseweg 297, 3731 GA De Bilt, the Netherlands

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Wim Van Westrenen,

Department of Earth Sciences, Vrije Universiteit, De Boelelaan 1085, 1081 HV Amsterdam, the Netherlands

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Michael E. Zolensky,

ARES, NASA Johnson Space Center, Mail Code XI2, Houston, Texas, 77058 USA

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Karen Ziegler,

Institute of Meteoritics, University of New Mexico, Albuquerque, New Mexico, 87131 USA

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Qing-Zhu Yin,

Department of Earth and Planetary Science, University of California Davis, One Shields Avenue, Davis, California, 95616 USA

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Matthew E. Sanborn,

Department of Earth and Planetary Science, University of California Davis, One Shields Avenue, Davis, California, 95616 USA

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Josh Wimpenny,

Department of Earth and Planetary Science, University of California Davis, One Shields Avenue, Davis, California, 95616 USA

Lawrence Livermore National Laboratory, 7000 East Ave, Livermore, California, 94550 USA

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Akane Yamakawa,

Department of Earth and Planetary Science, University of California Davis, One Shields Avenue, Davis, California, 95616 USA

National Institute of Environmental Studies, 16-2 Onogawa, Tsukuba-City, Ibaraki, 305-8506 Japan

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Sebastiaan J. De Vet,

Department of Research & Education, Naturalis Biodiversity Center, Darwinweg 2, 2333 CR Leiden, the Netherlands

Meteor Section, Royal Netherlands Association for Meteorology and Astronomy, Asmansweg 50, 2571 BK Den Haag, the Netherlands

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Matthias M. M. Meier,

Naturmuseum St. Gallen, Rorschacherstrasse 263, CH-9016 St. Gallen, Switzerland

Institute of Geochemistry and Petrology, ETH Zürich, CH-8092, Zürich, Switzerland

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Kees C. Welten,

Space Sciences Laboratory, University of California Berkeley, 7 Gauss Way, Berkeley, California, 94720 USA

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Kunihiko Nishiizumi,

Space Sciences Laboratory, University of California Berkeley, 7 Gauss Way, Berkeley, California, 94720 USA

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Marc W. Caffee,

Department of Earth, Atmospheric and Planetary Sciences and Department of Physics and Astronomy, Purdue University, West Lafayette, Indiana, 47907 USA

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Aaron S. Burton,

ARES, NASA Johnson Space Center, Mail Code XI2, Houston, Texas, 77058 USA

Solar System Exploration Division, NASA Goddard Space Flight Center, Greenbelt, Maryland, 20771 USA

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Jason P. Dworkin,

Solar System Exploration Division, NASA Goddard Space Flight Center, Greenbelt, Maryland, 20771 USA

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Daniel P. Glavin,

Solar System Exploration Division, NASA Goddard Space Flight Center, Greenbelt, Maryland, 20771 USA

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Qinghao Wu,

Department of Chemistry, Stanford University, Zare Lab, Stanford, California, 94305 USA

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Richard N. Zare,

Helmholtz Zentrum Munich, Ingolstaedter Landstrasse 1, D-86764 Neuherberg, Germany

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Alexander Ruf,

Helmholtz Zentrum Munich, Ingolstaedter Landstrasse 1, D-86764 Neuherberg, Germany

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Mourad Harir,

Department of Chemistry, Stanford University, Zare Lab, Stanford, California, 94305 USA

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Philippe Schmitt-Kopplin,

Helmholtz Zentrum Munich, Ingolstaedter Landstrasse 1, D-86764 Neuherberg, Germany

Technische Universität Muenchen, Maximus-von-Imhof-Forum 2, 85354 Freising, Germany

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The Diepenveen Meteorite Consortium,
First published: 13 May 2019
Citations: 3

Abstract

A carbonaceous chondrite was recovered immediately after the fall near the village of Diepenveen in the Netherlands on October 27, 1873, but came to light only in 2012. Analysis of sodium and poly-aromatic hydrocarbon content suggests little contamination from handling. Diepenveen is a regolith breccia with an overall petrology consistent with a CM classification. Unlike most other CM chondrites, the bulk oxygen isotopes are extremely 16O rich, apparently dominated by the signature of anhydrous minerals, distributed on a steep slope pointing to the domain of intrinsic CM water. A small subset plots closer to the normal CM regime, on a parallel line 2 ‰ lower in δ17O. Different lithologies in Diepenveen experienced varying levels of aqueous alteration processing, being less aqueously altered at places rather than more heated. The presence of an agglutinate grain and the properties of methanol-soluble organic compounds point to active impact processing of some of the clasts. Diepenveen belongs to a CM clan with ~5 Ma CRE age, longer than most other CM chondrites, and has a relatively young K-Ar resetting age of ~1.5 Ga. As a CM chondrite, Diepenveen may be representative of samples soon to be returned from the surface of asteroid (162173) Ryugu by the Hayabusa2 spacecraft.

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