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Impact conditions required for formation of melt by jetting in silicatesIt is demonstrated that the process of jetting which occurs when particles collide at oblique angles may produce melt at much lower velocities than are required for melt production in head-on collisions. The minimum velocities of impact required for jetting in aluminum, bronzitite, dunite, and quartz are calculated by the method of shock polars. The analysis, which depends on stated assumptions about attained pressures and the occurrence of jetting, uses shock-velocity particle-velocity equations of state with three shock regimes. The treatment indicates that jetting should arise in bronzitite, dunite, and quartz at relative velocities as low as 1-2 km/sec. At such velocities material which passes near the stagnation point in the jet-forming region is subjected to sufficiently high pressures so that it is probably melted.
Document ID
19780060156
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Kieffer, S. W.
(California, University Los Angeles, Calif., 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
Location: Flagstaff, AZ
Start Date: September 13, 1976
End Date: September 17, 1976
Accession Number
78A44065
Funding Number(s)
CONTRACT_GRANT: NSG-7052
Distribution Limits
Public
Copyright
Other

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