Further evidence for an impact origin of the Tsenkher structure in the Gobi-Altai, Mongolia

Geology of a 3.7 km crater with a well-preserved ejecta blanket

Goro Komatsu, Jens Ormö, Togookhuu Bayaraa, Tomoko Arai, Keisuke Nagao, Yoshihiro Hidaka, Naoki Shirai, Mitsuru Ebihara, Carl Alwmark, Lkhagva Gereltsetseg, Shoovdor Tserendug, Kazuhisa Goto, Takafumi Matsui, Sodnomsambuu Demberel

Research output: Contribution to journalReview article

Abstract

The Tsenkher structure in the Gobi-Altai, Mongolia is a c. 3.7 km diameter crater with a well-preserved ejecta blanket. It has been hypothesized to be either of impact or volcanic origin in our previous work. Observations during our 2007 expedition and related sample analyses give further support for an impact origin. The evidence includes the presence of a structurally uplifted near-circular rim surrounded by an ejecta blanket, and abundant breccias, some of which are melt- A nd millimetre-scale spherule-bearing. Planar deformation features (PDFs) were found in one quartz grain in a breccia sample. Fe-rich grains are found in a vesicular melt sample that is also characterized by elevated platinum group element (PGE) abundances with respect to the sedimentary bedrock of the area (approximately an order of magnitude). Noble gas analysis of one breccia sample yielded an elevated 3He/4He value of (5.0±0.2) × 10-6. Although not conclusive alone, these geochemical results are consistent with a contribution of meteoritic components. A volcanic origin, in particular a maar formation, would require explanations for the unusual conditions associated with Tsenkher, including its large size occurring in isolation, the structurally uplifted rim and the lack of a bedded base surge deposit. A pronounced rampart structure observed at the eastern ejecta is also unusual for any volcanic origin. 40Ar-39Ar dating of a vesicular melt sample gives an age of the Tsenkher structure of 4.9±0.9 Ma. The rampart structure could provide insights into the formation of similar ejecta morphologies associated with numerous impact craters on Mars.

Original languageEnglish
Pages (from-to)1-24
Number of pages24
JournalGeological Magazine
Volume156
Issue number1
DOIs
Publication statusPublished - 2019 Jan 1
Externally publishedYes

Fingerprint

ejecta
crater
geology
melt
breccia
maar
spherule
noble gas
platinum group element
Mars
bedrock
quartz

Keywords

  • breccia
  • ejecta
  • impact crater
  • maar
  • Mongolia
  • raised rim
  • Tsenkher

ASJC Scopus subject areas

  • Geology

Cite this

Further evidence for an impact origin of the Tsenkher structure in the Gobi-Altai, Mongolia : Geology of a 3.7 km crater with a well-preserved ejecta blanket. / Komatsu, Goro; Ormö, Jens; Bayaraa, Togookhuu; Arai, Tomoko; Nagao, Keisuke; Hidaka, Yoshihiro; Shirai, Naoki; Ebihara, Mitsuru; Alwmark, Carl; Gereltsetseg, Lkhagva; Tserendug, Shoovdor; Goto, Kazuhisa; Matsui, Takafumi; Demberel, Sodnomsambuu.

In: Geological Magazine, Vol. 156, No. 1, 01.01.2019, p. 1-24.

Research output: Contribution to journalReview article

Komatsu, G, Ormö, J, Bayaraa, T, Arai, T, Nagao, K, Hidaka, Y, Shirai, N, Ebihara, M, Alwmark, C, Gereltsetseg, L, Tserendug, S, Goto, K, Matsui, T & Demberel, S 2019, 'Further evidence for an impact origin of the Tsenkher structure in the Gobi-Altai, Mongolia: Geology of a 3.7 km crater with a well-preserved ejecta blanket', Geological Magazine, vol. 156, no. 1, pp. 1-24. https://doi.org/10.1017/S0016756817000620
Komatsu, Goro ; Ormö, Jens ; Bayaraa, Togookhuu ; Arai, Tomoko ; Nagao, Keisuke ; Hidaka, Yoshihiro ; Shirai, Naoki ; Ebihara, Mitsuru ; Alwmark, Carl ; Gereltsetseg, Lkhagva ; Tserendug, Shoovdor ; Goto, Kazuhisa ; Matsui, Takafumi ; Demberel, Sodnomsambuu. / Further evidence for an impact origin of the Tsenkher structure in the Gobi-Altai, Mongolia : Geology of a 3.7 km crater with a well-preserved ejecta blanket. In: Geological Magazine. 2019 ; Vol. 156, No. 1. pp. 1-24.
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abstract = "The Tsenkher structure in the Gobi-Altai, Mongolia is a c. 3.7 km diameter crater with a well-preserved ejecta blanket. It has been hypothesized to be either of impact or volcanic origin in our previous work. Observations during our 2007 expedition and related sample analyses give further support for an impact origin. The evidence includes the presence of a structurally uplifted near-circular rim surrounded by an ejecta blanket, and abundant breccias, some of which are melt- A nd millimetre-scale spherule-bearing. Planar deformation features (PDFs) were found in one quartz grain in a breccia sample. Fe-rich grains are found in a vesicular melt sample that is also characterized by elevated platinum group element (PGE) abundances with respect to the sedimentary bedrock of the area (approximately an order of magnitude). Noble gas analysis of one breccia sample yielded an elevated 3He/4He value of (5.0±0.2) × 10-6. Although not conclusive alone, these geochemical results are consistent with a contribution of meteoritic components. A volcanic origin, in particular a maar formation, would require explanations for the unusual conditions associated with Tsenkher, including its large size occurring in isolation, the structurally uplifted rim and the lack of a bedded base surge deposit. A pronounced rampart structure observed at the eastern ejecta is also unusual for any volcanic origin. 40Ar-39Ar dating of a vesicular melt sample gives an age of the Tsenkher structure of 4.9±0.9 Ma. The rampart structure could provide insights into the formation of similar ejecta morphologies associated with numerous impact craters on Mars.",
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AU - Ormö, Jens

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AU - Arai, Tomoko

AU - Nagao, Keisuke

AU - Hidaka, Yoshihiro

AU - Shirai, Naoki

AU - Ebihara, Mitsuru

AU - Alwmark, Carl

AU - Gereltsetseg, Lkhagva

AU - Tserendug, Shoovdor

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AU - Matsui, Takafumi

AU - Demberel, Sodnomsambuu

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N2 - The Tsenkher structure in the Gobi-Altai, Mongolia is a c. 3.7 km diameter crater with a well-preserved ejecta blanket. It has been hypothesized to be either of impact or volcanic origin in our previous work. Observations during our 2007 expedition and related sample analyses give further support for an impact origin. The evidence includes the presence of a structurally uplifted near-circular rim surrounded by an ejecta blanket, and abundant breccias, some of which are melt- A nd millimetre-scale spherule-bearing. Planar deformation features (PDFs) were found in one quartz grain in a breccia sample. Fe-rich grains are found in a vesicular melt sample that is also characterized by elevated platinum group element (PGE) abundances with respect to the sedimentary bedrock of the area (approximately an order of magnitude). Noble gas analysis of one breccia sample yielded an elevated 3He/4He value of (5.0±0.2) × 10-6. Although not conclusive alone, these geochemical results are consistent with a contribution of meteoritic components. A volcanic origin, in particular a maar formation, would require explanations for the unusual conditions associated with Tsenkher, including its large size occurring in isolation, the structurally uplifted rim and the lack of a bedded base surge deposit. A pronounced rampart structure observed at the eastern ejecta is also unusual for any volcanic origin. 40Ar-39Ar dating of a vesicular melt sample gives an age of the Tsenkher structure of 4.9±0.9 Ma. The rampart structure could provide insights into the formation of similar ejecta morphologies associated with numerous impact craters on Mars.

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