Shock Melting of the Canyon Diablo Impactor: Constraints from Nickel-59 Contents and Numerical Modeling
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Schnabel, C
Pierazzo, E
Xue, S
Herzog, G
Masarik, J
Cresswell, Richard
di Tada, M.
Liu, K.
Fifield, L Keith
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American Association for the Advancement of Science
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.
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2037-12-31
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