Shock melting of the Canyon Diablo impactor: Constraints from nickel-59 contents and numerical modeling

C. Schnabel, E. Pierazzo, S. Xue, G. F. Herzog*, J. Masarik, R. G. Cresswell, M. L. Di Tada, K. Liu, L. K. Fifield

*Corresponding author for this work

    Research output: Contribution to journalArticlepeer-review

    15 Citations (Scopus)

    Abstract

    Two main types of material survive from the Canyon Diablo impactor, which produced Meteor Crater in Arizona: iron meteorites, which did not melt during the impact; and spheroids, which did. Ultrasensitive measurements using accelerator mass spectrometry show that the meteorites contain about seven times as much nickel-59 as the spheroids. Lower average nickel-59 contents in the spheroids indicate that they typically carne from 0.5 to 1 meter deeper in the impactor than did the meteorites. Numerical modeling for an impact velocity of 20 kilometers per second shows that a shell 1.5 to 2 meters thick, corresponding to 16 percent of the projectile volume remained solid on the rear surface; that most of the projectile melted; and that little, if any, vaporized.

    Original languageEnglish
    Pages (from-to)85-88
    Number of pages4
    JournalScience
    Volume285
    Issue number5424
    DOIs
    Publication statusPublished - 2 Jul 1999

    Fingerprint

    Dive into the research topics of 'Shock melting of the Canyon Diablo impactor: Constraints from nickel-59 contents and numerical modeling'. Together they form a unique fingerprint.

    Cite this