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Impact-induced melting of planetary surfaces

O'Keefe, John D. and Ahrens, Thomas J. (1994) Impact-induced melting of planetary surfaces. In: Large Meteorite Impacts and Planetary Evolution. Special papers (Geological Society of America). No.293. Geological Society of America , Boulder, CO, pp. 103-109. ISBN 9780813722931. https://resolver.caltech.edu/CaltechAUTHORS:20150225-132357523

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Abstract

The objective of this paper is to determine the thickness of the melt layer relative to the crater diameter for simple and complex craters. A numerical code was employed to calculate the amount of melting and the crater geometry. We used the code results and the scaling formalism of Holsapple and Schmidt (1987) to determine the scaling laws for the relative melt layer thickness. Simple crater dimensions are dominated by impact parameters and the planet’s strength, whereas complex crater dimensions are dominated by planetary gravity, strength, and the impact parameters. The volume of melt is proportional to impact energy for impact velocities and melt enthalpies of interest to planetary science. Crater geometry and dimensions scale with an exponent, μ, which is intermediate between momentum (μ = 1/3) and energy (μ = 2/3) scaling. For simple craters, the melt layer thickness/crater diameter, T/D, for a given planetary surface (constant melt enthalpy and mean impact velocity), is independent of the crater size. For complex craters, T/D, for a given planetary surface (constant melt enthalpy, impact velocity, and gravitational acceleration), increases with the size of the crater. For simple craters, at a fixed size, the relative melt layer thickness, T/D, increases slowly with increasing impact velocity, U, according to ∝ U^(0.1)), whereas, for complex craters (∝ U^(0.22)).


Item Type:Book Section
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1130/SPE293-p103DOIArticle
http://specialpapers.gsapubs.org/content/293/103PublisherArticle
Additional Information:© 1994 Geological Society of America. Manuscript accepted by the Society December 28, 1993. Research supported under NASA grant NAGW 1953. We appreciate the assistance of Michael Lainhart with the calculations. We thank W. W. Anderson for comments on the manuscript. This chapter is Contribution 5259, Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, California.
Funders:
Funding AgencyGrant Number
NASANAGW 1953
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Other Numbering System NameOther Numbering System ID
Caltech Division of Geological and Planetary Sciences5259
Series Name:Special papers (Geological Society of America)
Issue or Number:293
Record Number:CaltechAUTHORS:20150225-132357523
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20150225-132357523
Official Citation:Processes and Effects of Impact Cratering: John D. O’Keefe and Thomas J. Ahrens Impact-induced melting of planetary surfaces Geological Society of America Special Papers, 1992, 293, p. 103-110, doi:10.1130/SPE293-p103
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:55197
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:26 Feb 2015 04:04
Last Modified:03 Oct 2019 08:03

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