• Search Research Projects
  • Search Researchers
  • How to Use
  1. Back to previous page

Origin and evolutionary processes of small mineral grains in the primitive meteorite matrix

Research Project

Project/Area Number 09440187
Research Category

Grant-in-Aid for Scientific Research (B)

Allocation TypeSingle-year Grants
Section一般
Research Field Petrology/Mineralogy/Science of ore deposit
Research InstitutionKobe University

Principal Investigator

TOMEOKA Kazushige  Kobe Univ., Science, Professor, 理学部, 教授 (00201658)

Co-Investigator(Kenkyū-buntansha) KOJIMA Tomoko  Kobe Univ., Science, Assistant, 理学部, 助手 (80281137)
Project Period (FY) 1997 – 1999
Project Status Completed (Fiscal Year 1999)
Budget Amount *help
¥12,400,000 (Direct Cost: ¥12,400,000)
Fiscal Year 1999: ¥1,300,000 (Direct Cost: ¥1,300,000)
Fiscal Year 1998: ¥1,300,000 (Direct Cost: ¥1,300,000)
Fiscal Year 1997: ¥9,800,000 (Direct Cost: ¥9,800,000)
KeywordsCarbonaceous chondrite / dark inclusion / chondrule rim / aqueous alteration / thermal matamorphism / shock metamorphism / fluidization / dehydration / 暗色包有物 / コンドリュール / 層状ケイ酸塩 / 普通コンドライト / 衝撃実験 / 小惑星 / 隕石母天体 / 皿状構造 / 衝撃変成作用
Research Abstract

(1)A dark inclusion in the Vigarano CV3 carbonaceous chondrite consists almost exclusively of small (<5 μm in diameter) grains of Fe-rich olivine. This dark inclusion shows an unusual texture comprising a network of arcuate bands. Two or more bands occur roughly parallel, forming a set of succesive parallel bands, some crosscutting one another. The bands contain slightly higher amounts of relatively small (<1 μm) olivine grains and so are more densely packed than other areas. The olivine grains in the bands are slightly more Fe-rich than those in other areas. The bands commonly show gradation on the concave side due to a decrease in the abundance of the small Fe-rich olivine grains. Texturally, the arcuate bands closely resemble "dish structures" that are commonly observed in siltstones and sandstones on Earth. Dish structures are characterized by thin, dark-colored, subhorizontal to concave-upward laminations which are rich in relatively fine-grained material. On Earth, dish structure … More s from during compaction and dewatering of unconsolidated fine-grained sediments and they are one of the characteristic sedimentary structures formed through fluidization of fine grains. The dark inclusion in Vigarano, therefore, provides the first evidence that sedimentary processes due to water migration may have taken place within planetesimals, and further suggests that fluidization may have played a significant role in the formation of the carbonaceous chondrites.
(2)The results of a series of shock experiments on the Murchison Cm chondrite reveal that chondrules are flattened in the plane of the shock front roughly in proportion to the intensity of peak shock pressure up to 〜25 GPa, but at 25-30 GPa they are no longer flattened but are increasingly disrupted. Changes involving fracturing and comminution begin to occur in matrix at 〜20 GPa, and these changes drastically advance with increasing pressure between 25 and 30 GPa ; thus, the matrix is densely comminuted on scales of 10-50 μm. Local melting also occurs as melt veins and pockets at 20-30 GPa. At pressures higher than 30-35 GPa, Murchison responds to shock with catastrophic disruption accompanied by extensive melting, fragmentation, pulverization, devolatilization and intense expansion of gas. Our calculations of internal energy increase upon impact suggest that the shock thermal effects produced at each experiment may be attained by impact on a natural target (surface material in the Murchison parent body) at a considerably lower shock pressure than the peak shock pressure. These results suggest that if the CM parent body were shocked on the surface at pressures higher than 〜25 GPa, on pressure release there would be explosive dispersal of fine grains, and water and mobilized volatiles would escape with these grains from the parent body. Therefore, the results support the hypothesis that CM chondrites shocked above 20-30 GPa escaped from the parent asteroids and formed particles that are too small to survive as meteorites. This probably explains why we have no CM chondrites shocked to the stages higher than S3 levels. It may also provide a clue to the long-standing question of why the most chemically primitive meteorite falls, such as CI and CM chondrites, are relatively few, while among the main belt asteroids those classified as C-type are abundant.
(3)The vast majority of previous workers favor that fine-grained rims surrounding chondrules are primitive in origin and formed by direct accretion of dust onto the surfaces of chondrules and CAIs in the solar nebula. Recently, we found that a small proportion (〜5%) of the fine-grained rims surrounding chondrules in the Vigarano CV3 chondrite consists mainly of hydrous phyllosilicates. The phyllosilicate-rich rims and the chondrules that they enclose show abundant evidence of aqueous alteration. Low-Ca pyroxene and olivine at chondrule margins have been partially replaced by phyllosilicate-rich materials, producing embayments on chondrule surfaces. Fe-Ni metal, Fe sulfide and magnetite in the chondrules have also been partially replaced by Fe hydroxide. Due to preferential replacement of low-Ca pyroxene and olivine, sulfide, magnetic and Fe hydroxide remain exposed at chondrule margins and are partly disaggregated an distributed into rims. The mineralogical and textural evidence can not be reconciled with rim formation by accretion in the solar nebula but can be most plausible explained by aqueous alteration and brecciation on the meteorite parent body. From these observations, we suggest that the chondrule/rim assemblages and the clasts are a part of the same precursor chondrite, which was fragmented during brecciation on the meteorite parent body. This is the first self-consistent model to explain the formation of fine-grained rims on chondrules in a carbonaceous chondrite by parent-body processes. This work is still in progress. Less

Report

(4 results)
  • 1999 Annual Research Report   Final Research Report Summary
  • 1998 Annual Research Report
  • 1997 Annual Research Report
  • Research Products

    (25 results)

All Other

All Publications (25 results)

  • [Publications] T. Kojima: "A fine-grained dark inclusion in the Vigarano CV3 chondrite : record of accumulation processes on the meteorite parent body"Antarctic Meteorite Research. 10. 203-215 (1997)

    • Description
      「研究成果報告書概要(和文)」より
    • Related Report
      1999 Final Research Report Summary
  • [Publications] K. Tomeoka: "Arcuate band texture in a dark inclusion from the Vigarano CV3 chondrite : Possible evidence for early sedimentary processes"Meteoritics & Planetary Science. 33. 519-525 (198)

    • Description
      「研究成果報告書概要(和文)」より
    • Related Report
      1999 Final Research Report Summary
  • [Publications] K. Tomeoka: "Experimental shock metamorphism of the Murchison CM carbonaceous chondrite"Geochimica et Cosmochinica Acta. 63. 3683-3703 (1999)

    • Description
      「研究成果報告書概要(和文)」より
    • Related Report
      1999 Final Research Report Summary
  • [Publications] K. Tomeoka: "Phyllosilicate-rich chondrule rims in the Vigarano CV2 chondrite : Evidence for parent-body processes"Geochimica et Cosmochinica Acta. 64 (印刷中). (2000)

    • Description
      「研究成果報告書概要(和文)」より
    • Related Report
      1999 Final Research Report Summary
  • [Publications] T. Nakamura: "Impact-induced textural and compositional changes of CV carbonaceous chondrites : Experimental reproduction"Icarus. (印刷中). (2000)

    • Description
      「研究成果報告書概要(和文)」より
    • Related Report
      1999 Final Research Report Summary
  • [Publications] T. Kojima: "A dark inclusion in the Maynch LL (3.1) ordinary chondrite : A Product of strong shock metamorphism"Antarctic Meteorite Research. 13 (印刷中). (2000)

    • Description
      「研究成果報告書概要(和文)」より
    • Related Report
      1999 Final Research Report Summary
  • [Publications] T.Kojima and K.Tomeoka: "A fine-grained dark inclusion in the Vigarano CV3 chondrite : record of accumulation processes on the meteorite parent body"Proc. National Institute of Polar Research Symposium on Antarctic Meteorites. 10. 203-215 (1997)

    • Description
      「研究成果報告書概要(欧文)」より
    • Related Report
      1999 Final Research Report Summary
  • [Publications] K.Tomeoka: "Aqueous alteration and dehydration processes in the carbonaceous chondrites""Parent-body and Nebular Modification of Chondritic Materials", Lunar & Planetary Institute Technical Report. 2. 61-62 (1997)

    • Description
      「研究成果報告書概要(欧文)」より
    • Related Report
      1999 Final Research Report Summary
  • [Publications] K. Tomeoka, Y.Yamahana and T.Sekine: "Shock effects of a carbonaceous chondrite meteorite : an experimental study"Proc. NIRIM Interna. Symp. Advanced Materials. 5. 205-208 (1998)

    • Description
      「研究成果報告書概要(欧文)」より
    • Related Report
      1999 Final Research Report Summary
  • [Publications] K.Tomeoka and T.Kojima: "Arcuate band texture in a dark inclusion from the Vigarano CV3 chondrite : Possible evidence for early sedimentary processes"Meteoritics & Planetary Science. 33. 519-525 (1998)

    • Description
      「研究成果報告書概要(欧文)」より
    • Related Report
      1999 Final Research Report Summary
  • [Publications] K.Tomeoka, Y.Yamahana and T.Sekine: "Experimental shock metamorphism of the Murchison CM carbonaceous chondrite"Geochimica et Cosmochimica Acta. 63. 3683-3703 (1999)

    • Description
      「研究成果報告書概要(欧文)」より
    • Related Report
      1999 Final Research Report Summary
  • [Publications] T.Kojima, T.Yatagai and K.Tomeoka: "A dark inclusion in the Maynch LL(3.1) ordinary chondrite : A product of strong shock metamorphism"Antarctic Meteorite Research. 13(in press).

    • Description
      「研究成果報告書概要(欧文)」より
    • Related Report
      1999 Final Research Report Summary
  • [Publications] T.Nakamura, K.Tomeoka, N.Takaoka, T.Sekine and H.Takeda: "Impact-induced textural and compositional changes of CV carbonaceous chondrites : Experimental reproduction"Icarus. (in press).

    • Description
      「研究成果報告書概要(欧文)」より
    • Related Report
      1999 Final Research Report Summary
  • [Publications] K.Tomeoka and I.Tanimura: "Phyllosilicate-rich chondrule rims in the Vigarano CV3 chondrite : Evidence for parent-body processes"Geochimica et Cosmochimica Acta. 64(in press).

    • Description
      「研究成果報告書概要(欧文)」より
    • Related Report
      1999 Final Research Report Summary
  • [Publications] K.Tomeoka: "Experimental shock metamorphism of the Murchison CM carbonaceous chondrite"Geochimica et Cosmochimica Acta. 63. 3683-3703 (1999)

    • Related Report
      1999 Annual Research Report
  • [Publications] K.Tomeoka: "Phyllosilicate-rich chondrule rims in the Vigarano CV3 chondrite: Evidence for parent-body processes"Geochimica et Cosmochimica Acta. 64(印刷中). (2000)

    • Related Report
      1999 Annual Research Report
  • [Publications] T.Nakamura: "Impact-induced textural and compositional changes of CV carbonaceous chondrites: Experimental reproduction"Icarus. (印刷中). (2000)

    • Related Report
      1999 Annual Research Report
  • [Publications] T.Kojima: "A dark inclusion in the Maynch LL(3.1) ordinary chondrite: A product of strong shock metamorphism"Antarctic Meteorite Research. (印刷中). (2000)

    • Related Report
      1999 Annual Research Report
  • [Publications] K.Tomeoka: "Arcuate band texture in a dark inclusion from the Vigarano CV3 chondrite : possible evience for early sedimentary processes" Meteoritics & Planetary Science. 33. 519-525 (1998)

    • Related Report
      1998 Annual Research Report
  • [Publications] K.Tomeoka: "Shock effects of a carbonaceous chondrite meteorite : an experimental study" Proc.NIRIM International Symposium on Advanced Materials. 5. 205-208 (1998)

    • Related Report
      1998 Annual Research Report
  • [Publications] K.Tomeoka: "Experimental shock metamorphism of the Murchison CM carbonaceous chondrite" Geochimica et Cosmochimica Acta. (発表予定). (1999)

    • Related Report
      1998 Annual Research Report
  • [Publications] T.Kojima: "A fine-grained dark inclusion in the Vigarano CV3 chondrite : possible evidence for sedimentary process on the meterite parent body," Antarctic Meteorite Research. 10. 203-215 (1997)

    • Related Report
      1997 Annual Research Report
  • [Publications] K.Tomeoka: "Aqueous alteration and dehydration processes in the carbonaceous chondrites" Lunar & Planetary Institute Technical Report “Parent-body and Nebular Modification of Chondritic Materials". 61-62 (1997)

    • Related Report
      1997 Annual Research Report
  • [Publications] K.Tomeoka: "Shock effects of a carbonaceous chondrite meteorite : an experimental study" Proc.NIRIM International Symposium on Advanced Materials. 5. 205-208 (1998)

    • Related Report
      1997 Annual Research Report
  • [Publications] K.Tomeoka: "Arcuate band texture in a dark inclusion from the Vigarano CV3 chondrite : possible evience for early sedimentary processes" Meteoritics & Planetary Science. (印刷中). (1998)

    • Related Report
      1997 Annual Research Report

URL: 

Published: 1997-04-01   Modified: 2016-04-21  

Information User Guide FAQ News Terms of Use Attribution of KAKENHI

Powered by NII kakenhi