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Buffering of diurnal temperature variations on Venus
Authors:Bruce M Jakosky
Institution:Laboratory for Atmospheric and Space Physics, University of Colorado, Boulder, Colorado 80309, USA
Abstract:Previous calculations of the role of degassing of CO2 from calcite in buffering the surface temperature of Venus ignored the efficacy with which energy could be conducted into the subsurface. Consuction into the subsurface plays a minor role in the energy balance, however, such that less than 10% of the insolation will conduct into the subsurface and go into degassing CO2, with the remainder heating up the surface and atmosphere; negligible buffering of the surface temperature will occur.
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