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Proceedings of the Japan Academy Series B: Physical and Biological SciencesVolume 95, Issue 4, 2019, Pages 165-177

Hypervelocity collision and water-rock interaction in space preserved in the Chelyabinsk ordinary chondrite(Article)(Open Access)

  • Nakamura, E.,
  • Kunihiro, T.,
  • Ota, T.,
  • Sakaguchi, C.,
  • Tanaka, R.,
  • Kitagawa, H.,
  • Kobayashi, K.,
  • Yamanaka, M.,
  • Shimaki, Y.,
  • Bebout, G.E.,
  • Miura, H.,
  • Yamamoto, T.,
  • Malkovets, V.,
  • Grokhovsky, V.,
  • Koroleva, O.,
  • Litasov, K.
  • View Correspondence (jump link)
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  • aThe Pheasant Memorial Laboratory for Geochemistry and Cosmochemistry, Institute for Planetary Materials, Okayama University, Tottori, Japan
  • bDepartment of Earth and Environmental Sciences, Lehigh University, Bethlehem, PA, United States
  • cGraduate School of Natural Sciences, Nagoya City University, Nagoya, Japan
  • dInstitute of Low Temperature Science, Hokkaido University, Sapporo, Japan
  • eInstitute of Physics and Technology, Ural Federal University, Yekaterinburg, Russian Federation
  • fInstitute of Mineralogy, Ural Branch of the Russian Academy of Sciences, Miass, Russian Federation
  • gSouth-Ural State University, Chelyabinsk, Russian Federation
  • hV.S. Sobolev Institute of Geology and Mineralogy, Siberian Branch of the Russian Academy of Sciences, Novosibirsk, Russian Federation

Abstract

A comprehensive geochemical study of the Chelyabinsk meteorite reveals further details regarding its history of impact-related fragmentation and melting, and later aqueous alteration, during its transit toward Earth. We support an 930Ma age obtained by Ar-Ar method (Beard et al., 2014) for the impact-related melting, based on Rb-Sr isotope analyses of a melt domain. An irregularly shaped olivine with a distinct O isotope composition in a melt domain appears to be a fragment of a silicate-rich impactor. Hydrogen and Li concentrations and isotopic compositions, textures of Fe oxyhydroxides, and the presence of organic materials located in fractures, are together consistent with aqueous alteration, and this alteration could have pre-dated interaction with the Earth's atmosphere. As one model, we suggest that hypervelocity capture of the impact-related debris by a comet nucleus could have led to shock-wave-induced supercritical aqueous fluids dissolving the silicate, metallic, and organic matter, with later ice sublimation yielding a rocky rubble pile sampled by the meteorite. © 2019 The Japan Academy.

Author keywords

AsteroidChronologyCometGeochemistryImpact meltingOrdinary chondrite

Indexed keywords

EMTREE drug terms:water
EMTREE medical terms:astronomychemistry
MeSH:Earth (Planet)Evolution, PlanetaryMeteoroidsWater

Chemicals and CAS Registry Numbers:

water, 7732-18-5;

Water

Funding details

Funding sponsor Funding number Acronym
Japan Society for the Promotion of Science
See opportunities by JSPS
16K05578,17K05706JSPS
Japan Society for the Promotion of Science
See opportunities by JSPS
JSPS
  • ISSN: 03862208
  • Source Type: Journal
  • Original language: English
  • DOI: 10.2183/pjab.95.013
  • PubMed ID: 30971619
  • Document Type: Article
  • Publisher: Japan Academy

  Nakamura, E.; The Pheasant Memorial Laboratory for Geochemistry and Cosmochemistry, Institute for Planetary Materials, Okayama University, 827 Yamada, Misasa, Tottori, Japan;
© Copyright 2019 Elsevier B.V., All rights reserved.

Cited by 8 documents

Chen, C. , Yi, R. , Igisu, M.
Spectroscopic and Biophysical Methods to Determine Differential Salt-Uptake by Primitive Membraneless Polyester Microdroplets
(2023) Small Methods
Ota, T. , Potiszil, C. , Kobayashi, K.
The Formation of a Rubble Pile Asteroid: Insights from the Asteroid Ryugu
(2023) Universe
Beard, S.P. , Swindle, T.D. , Lapen, T.J.
Ar-Ar and U-Pb ages of Chelyabinsk and a re-evaluation of its impact chronology
(2022) Meteoritics and Planetary Science
View details of all 8 citations
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