Dynamical implications of the petrology and distribution of impact melt rocksPetrographic and structural relations of rocks resulting from melting of target materials during impact indicate constraints that can be applied to theoretical models and experimental production of craters. Topics discussed in this context include the motion of shock melted material, the mixing of melts, the energies required for heating and melting the necessary volumes of target rocks, diameter to depth ratios, and the formation of structural modifications. The motion of shock melted material involves ejection of some of the lowermost parts of the target, incorporation of distant fragmental material, outward flow, settling into cracks after breccia formation, and completion in a short time span. Melts must be completed within tens of seconds to a couple of minutes after impact.
Document ID
19780060157
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Phinney, W. C. (NASA Johnson Space Center Houston, Tex., United States)
Simonds, C. H. (Lunar and Planetary Institute Houston, Tex., United States)
Date Acquired
August 9, 2013
Publication Date
January 1, 1977
Subject Category
Lunar And Planetary Exploration
Meeting Information
Meeting: Symposium on Planetary Cratering Mechanics