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    Cubic zirconia in >2370 °C impact melt records Earth's hottest crust

    255643.pdf (13.59Mb)
    Access Status
    Open access
    Authors
    Timms, Nicholas Eric
    Erickson, T.
    Zanetti, M.
    Pearce, M.
    Cayron, C.
    Cavosie, Aaron
    Reddy, S.
    Wittmann, A.
    Carpenter, P.
    Date
    2017
    Type
    Journal Article
    
    Metadata
    Show full item record
    Citation
    Timms, N.E. and Erickson, T. and Zanetti, M. and Pearce, M. and Cayron, C. and Cavosie, A. and Reddy, S. et al. 2017. Cubic zirconia in >2370 °C impact melt records Earth's hottest crust. Earth and Planetary Science Letters. 477: pp. 52-58.
    Source Title
    Earth and Planetary Science Letters
    DOI
    10.1016/j.epsl.2017.08.012
    ISSN
    0012-821X
    School
    Department of Applied Geology
    URI
    http://hdl.handle.net/20.500.11937/57023
    Collection
    • Curtin Research Publications
    Abstract

    Bolide impacts influence primordial evolution of planetary bodies because they can cause instantaneous melting and vaporization of both crust and impactors. Temperatures reached by impact-generated silicate melts are unknown because meteorite impacts are ephemeral, and established mineral and rock thermometers have limited temperature ranges. Consequently, impact melt temperatures in global bombardment models of the early Earth and Moon are poorly constrained, and may not accurately predict the survival, stabilization, geochemical evolution and cooling of early crustal materials. Here we show geological evidence for the transformation of zircon to cubic zirconia plus silica in impact melt from the 28 km diameter Mistastin Lake crater, Canada, which requires super-heating in excess of 2370 °C. This new temperature determination is the highest recorded from any crustal rock. Our phase heritage approach extends the thermometry range for impact melts by several hundred degrees, more closely bridging the gap between nature and theory. Profusion of >2370 °C superheated impact melt during high intensity bombardment of Hadean Earth likely facilitated consumption of early-formed crustal rocks and minerals, widespread volatilization of various species, including hydrates, and formation of dry, rigid, refractory crust.

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