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Impact melt generation and transportThe results from the first two calculations in a series of continuum mechanics computer code calculations, investigating the effects of variations in impactor mass and velocity on the generation and transport of impact melt, are reported. In the present calculations, the impactor is modeled as a spherical iron projectile with a mass of one trillion grams, and the target as a gabbroic anorthosite (GA) half-space, where the cases calculated have impact velocities of 5 and 15.8 km/sec. Early-time ejection velocities are 1-2 km/sec in both cases. The first calculation results in 0.07 projectile masses of GA being partly or completely melted, with all the melted GA being ejected from the crater, and a maximum impact range for the ejected melted material of 30 km. The second calculation yields 10.4 projectile masses of melted GA, 50% of which is ejected from the crater to ranges of up to about 130 km. Peak shock pressure attenuation with depth is reported for both cases, and transient cavity dynamics are described and compared to that for surface and near-surface explosions.
Document ID
19820038851
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Orphal, D. L.
(California Research and Technology, Inc. Livermore, CA, United States)
Borden, W. F.
(California Research and Technology, Inc. Livermore, CA, United States)
Larson, S. A.
(California Research and Technology, Inc. Livermore, CA, United States)
Schultz, P. H.
(Lunar and Planetary Institute Houston, TX, United States)
Date Acquired
August 10, 2013
Publication Date
January 1, 1980
Subject Category
Lunar And Planetary Exploration
Meeting Information
Meeting: Lunar and Planetary Science Conference
Location: Houston, TX
Start Date: March 17, 1980
End Date: March 21, 1980
Accession Number
82A22386
Funding Number(s)
CONTRACT_GRANT: NSR-09-051-001
CONTRACT_GRANT: NASW-3276
Distribution Limits
Public
Copyright
Other

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