Dbj. Bussey et al., FACTORS INFLUENCING THE CAPABILITY OF LAVA TO ERODE ITS SUBSTRATE - APPLICATION TO VENUS, J GEO R-PLA, 100(E8), 1995, pp. 16941-16948
There is evidence that a uniquely Venusian type of channel may be at l
east partly erosional in origin. A number of published models discuss
the erosion process on various planetary bodies. However, these relate
to lavas of specifically different compositions. Here a numerical mod
el is derived to investigate the sensitivity of the erosion process to
various physical parameters of the lava and substrate, placing constr
aints on the physical characteristics required to obtain a suitably ra
pid erosion rate. The model allows for the effects of latent heat and
also considers the presence of a liquid substrate boundary layer betwe
en the lava and solid substrate. The results indicate that the thermal
erosion process is particularly sensitive to the melting temperature,
when the melting temperature is doubled from 700 to 1400 K, the erosi
on rate decreases by approximately an order of magnitude. Also, the er
osion rate associated with a venusian initial substrate temperature is
approximately 1.5 times greater than the equivalent terrestrial one.
Mechanical erosion is considered by altering the percentage of latent
heat required to melt the substrate; as this percentage is varied from
0 to 100, the erosion rate decreases by about a factor of 2.