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Impact-induced shock and the formation of natural quasicrystals in the early solar system

Author

Listed:
  • Lincoln S. Hollister

    (Princeton University, Guyot Hall)

  • Luca Bindi

    (Università di Firenze)

  • Nan Yao

    (Princeton Institute for the Science and Technology of Materials, Princeton University)

  • Gerald R. Poirier

    (Princeton Institute for the Science and Technology of Materials, Princeton University
    Present address: Advanced Material Characterization Laboratory, University of Delaware, Wilmington, North Carolina 19801, USA)

  • Christopher L. Andronicos

    (Purdue University)

  • Glenn J. MacPherson

    (National Museum of Natural History, Smithsonian Institution)

  • Chaney Lin

    (Princeton University, Jadwin Hall)

  • Vadim V. Distler

    (Institute of Geology of Ore Deposits, Petrography, Mineralogy, and Geochemistry (IGEM), Russian Academy of Sciences)

  • Michael P. Eddy

    (Atmospheric, and Planetary Sciences, Massachusetts Institute of Technology)

  • Alexander Kostin

    (Geoscience Technology, BHP Billiton)

  • Valery Kryachko

    (Institute of Geology of Ore Deposits, Petrography, Mineralogy, and Geochemistry (IGEM), Russian Academy of Sciences)

  • William M. Steinhardt

    (Harvard University)

  • Marina Yudovskaya

    (Institute of Geology of Ore Deposits, Petrography, Mineralogy, and Geochemistry (IGEM), Russian Academy of Sciences)

  • John M. Eiler

    (California Institute of Technology)

  • Yunbin Guan

    (California Institute of Technology)

  • Jamil J. Clarke

    (Hitachi High Technologies America, Inc.)

  • Paul J. Steinhardt

    (Princeton University, Jadwin Hall
    Princeton Center for Theoretical Science, Princeton University)

Abstract

The discovery of a natural quasicrystal, icosahedrite (Al63Cu24Fe13), accompanied by khatyrkite (CuAl2) and cupalite (CuAl) in the CV3 carbonaceous chondrite Khatyrka has posed a mystery as to what extraterrestrial processes led to the formation and preservation of these metal alloys. Here we present a range of evidence, including the discovery of high-pressure phases never observed before in a CV3 chondrite, indicating that an impact shock generated a heterogeneous distribution of pressures and temperatures in which some portions reached at least 5 GPa and 1,200 °C. The conditions were sufficient to melt Al–Cu-bearing minerals, which then rapidly solidified into icosahedrite and other Al–Cu metal phases. The meteorite also contains heretofore unobserved phases of iron–nickel and iron sulphide with substantial amounts of Al and Cu. The presence of these phases in Khatyrka provides further proof that the Al–Cu alloys are natural products of unusual processes that occurred in the early solar system.

Suggested Citation

  • Lincoln S. Hollister & Luca Bindi & Nan Yao & Gerald R. Poirier & Christopher L. Andronicos & Glenn J. MacPherson & Chaney Lin & Vadim V. Distler & Michael P. Eddy & Alexander Kostin & Valery Kryachko, 2014. "Impact-induced shock and the formation of natural quasicrystals in the early solar system," Nature Communications, Nature, vol. 5(1), pages 1-8, September.
  • Handle: RePEc:nat:natcom:v:5:y:2014:i:1:d:10.1038_ncomms5040
    DOI: 10.1038/ncomms5040
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