Mathematics
Scientific paper
Dec 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992lpico.789q..14b&link_type=abstract
In Lunar and Planetary Inst., Papers Presented to the International Colloquium on Venus p 14 (SEE N93-14288 04-91)
Mathematics
Cratering, Monte Carlo Method, Planetary Craters, Planetary Evolution, Three Dimensional Models, Topography, Venus (Planet), Volcanoes, Volcanology, Asteroids, Comets, Fluid Flow, Lava, Mass Distribution, Mathematical Models
Scientific paper
We have developed a three-dimensional model of venusian resurfacing that employs Monte Carlo simulations of both impact cratering and volcanism. The model simulates the production of craters on Venus by using the observed mass distributions of Earth- and Venus-crossing asteroids and comets. Lava flows are modeled by an energy minimization technique to simulate the effects of local topography on the shape and extent of flows. The model is run under a wide range of assumptions regarding the scale and time evolution of volcanism on Venus. Regions of the parameter space that result in impact crater distributions and modifications that are currently observed will be explored to place limits on the possible volcanic resurfacing history of Venus.
Bullock Mark Alan
Grinspoon David H.
Head James W. III
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