Forecast of the surface structure of moon, Mars, Mercury and Venus based on radio-astronomical observations of their thermal conditions

Details Forecast of the surface structure of moon, Mars, Mercury and Venus based on radio-astronomical observations of their thermal conditions Forecast of the surface structure of moon, Mars, Mercury and Venus based on radio-astronomical observations of their thermal conditions

Jul 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978ijhmt..21..827d&link_type=abstract

International Journal of Heat and Mass Transfer, vol. 21, July 1978, p. 827-834.

Astronomy and Astrophysics

Astronomy

1

Forecasting, Heat Transfer, Lunar Soil, Mars Surface, Mercury (Planet), Radio Astronomy, Surface Properties, Venus Surface, Optical Properties, Planetary Surfaces, Remote Sensors, Surface Layers, Temperature Distribution, Thermophysical Properties, Moon, Mars, Mercury, Venus, Earth, Surface, Soils, Structure, Radio Astronomy, Thermal Properties, Textures, Heat Flux, Radiation, Physical Properties, Observations

Scientific paper

Soil texture of planetary bodies is estimated by comparing observed and calculated values of a thermal parameter. The parameter is equal to the square root of the product of the effective thermal conductivity of the surface layer, the specific heat of the soil, and the volume density of the soil. Values of these soil parameters are adjusted until a thermal parameter value is achieved which equals the value determined by radio astronomical observations. Constraints on the plausible range of soil parameter values are based on consideration of the effects of soil characteristics and on information obtained by electrophysical and optical observations. The method is applied with respect to the moon, Mars, Mercury, and Venus.

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