Suevites and Tagamites of Zhamanshin Astrobleme

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Suevites and Tagamites of Zhamanshin Astrobleme : Distribution in the Crater and Petrographic Features. / Sergienko, E. S.; Yanson, S. Yu; Kosterov, A.; Kharitonskii, P. V.; Frolov, A. M.

In: IOP Conference Series: Earth and Environmental Science, Vol. 666, No. 4, 042080, 09.03.2021.

Research output: Contribution to journal › Conference article › peer-review

Author

Sergienko, E. S. ; Yanson, S. Yu ; Kosterov, A. ; Kharitonskii, P. V. ; Frolov, A. M. / Suevites and Tagamites of Zhamanshin Astrobleme : Distribution in the Crater and Petrographic Features. In: IOP Conference Series: Earth and Environmental Science. 2021 ; Vol. 666, No. 4.

BibTeX

@article{b1fe66e4eaf14228910240bcbcf83ac0,

title = "Suevites and Tagamites of Zhamanshin Astrobleme: Distribution in the Crater and Petrographic Features",

abstract = "The study of impact glasses from the Zhamanshin meteorite crater has a long history extending back to early 1970ies. Most attention is paid to unique impact-related rocks known as zhamanshinites (bombs) and irghizites (lapilli). But, as first shown by V.L. Masaitis, other, more common types of impactites, suevites and massive melts (tagamites), are also present in Zhamanshin. We study the distribution in the crater, structure and composition of these particular rocks using powder X-ray diffraction and scanning electron microscopy. It is shown that all impact glasses from the Zhamanshin crater are genetically related and derive from the impact event, while the observed petrographic differences between them reflect the conditions of their formation. Individual varieties of studied impactites (suevites and tagamites) are spatially separated and, as a rule, do not intersect. This points to the absence of global mixing of the target material as a result of the impact event, as well as to the complex nature of the impactor.",

author = "Sergienko, {E. S.} and Yanson, {S. Yu} and A. Kosterov and Kharitonskii, {P. V.} and Frolov, {A. M.}",

note = "Publisher Copyright: {\textcopyright} Published under licence by IOP Publishing Ltd. Copyright: Copyright 2021 Elsevier B.V., All rights reserved.; 2020 International Science and Technology Conference on Earth Science, ISTCEarthScience 2020 ; Conference date: 06-10-2020 Through 09-10-2020",

year = "2021",

month = mar,

day = "9",

doi = "10.1088/1755-1315/666/4/042080",

language = "English",

volume = "666",

journal = "IOP Conference Series: Earth and Environmental Science",

issn = "1755-1307",

publisher = "IOP Publishing Ltd.",

number = "4",

}

RIS

TY - JOUR

T1 - Suevites and Tagamites of Zhamanshin Astrobleme

T2 - 2020 International Science and Technology Conference on Earth Science, ISTCEarthScience 2020

AU - Sergienko, E. S.

AU - Yanson, S. Yu

AU - Kosterov, A.

AU - Kharitonskii, P. V.

AU - Frolov, A. M.

PY - 2021/3/9

Y1 - 2021/3/9

N2 - The study of impact glasses from the Zhamanshin meteorite crater has a long history extending back to early 1970ies. Most attention is paid to unique impact-related rocks known as zhamanshinites (bombs) and irghizites (lapilli). But, as first shown by V.L. Masaitis, other, more common types of impactites, suevites and massive melts (tagamites), are also present in Zhamanshin. We study the distribution in the crater, structure and composition of these particular rocks using powder X-ray diffraction and scanning electron microscopy. It is shown that all impact glasses from the Zhamanshin crater are genetically related and derive from the impact event, while the observed petrographic differences between them reflect the conditions of their formation. Individual varieties of studied impactites (suevites and tagamites) are spatially separated and, as a rule, do not intersect. This points to the absence of global mixing of the target material as a result of the impact event, as well as to the complex nature of the impactor.

AB - The study of impact glasses from the Zhamanshin meteorite crater has a long history extending back to early 1970ies. Most attention is paid to unique impact-related rocks known as zhamanshinites (bombs) and irghizites (lapilli). But, as first shown by V.L. Masaitis, other, more common types of impactites, suevites and massive melts (tagamites), are also present in Zhamanshin. We study the distribution in the crater, structure and composition of these particular rocks using powder X-ray diffraction and scanning electron microscopy. It is shown that all impact glasses from the Zhamanshin crater are genetically related and derive from the impact event, while the observed petrographic differences between them reflect the conditions of their formation. Individual varieties of studied impactites (suevites and tagamites) are spatially separated and, as a rule, do not intersect. This points to the absence of global mixing of the target material as a result of the impact event, as well as to the complex nature of the impactor.

UR - http://www.scopus.com/inward/record.url?scp=85102736209&partnerID=8YFLogxK

UR - https://www.mendeley.com/catalogue/6ea7b022-9d93-372e-aad8-aad54a0a8985/

U2 - 10.1088/1755-1315/666/4/042080

DO - 10.1088/1755-1315/666/4/042080

M3 - Conference article

AN - SCOPUS:85102736209

VL - 666

JO - IOP Conference Series: Earth and Environmental Science

JF - IOP Conference Series: Earth and Environmental Science

SN - 1755-1307

IS - 4

M1 - 042080

Y2 - 6 October 2020 through 9 October 2020

ER -

ID: 74885410