Solid state convection models of lunar internal temperature

Details Solid state convection models of lunar internal temperature Solid state convection models of lunar internal temperature

May 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975stin...7527991s&link_type=abstract

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Mathematics

Logic

Convective Heat Transfer, Lunar Geology, Lunar Temperature, Solid State, Creep Properties, Dynamic Models, Electrical Resistivity, Heat Flux, Lunar Seismographs

Scientific paper

Thermal models of the Moon were made which include cooling by subsolidus creep and consideration of the creep behavior of geologic material. Measurements from the Apollo program on seismic velocities, electrical conductivity of the Moon's interior, and heat flux at two locations were used in the calculations. Estimates of 1500 to 1600 K were calculated for the temperature, and one sextillion to ten sextillion sq cm/sec were calcualted for the viscosity of the deep lunar interior.

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