Microwave emission spectrum of the moon - Mean global heat flow and average depth of the regolith

Astronomy and Astrophysics – Astronomy

Scientific paper

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Brightness Temperature, Emission Spectra, Heat Flux, Lunar Temperature, Microwave Emission, Radio Spectra, Lunar Radiation, Lunar Surface, Radio Astronomy, Surface Layers

Scientific paper

Earth-based observations of the lunar microwave brightness temperature spectrum at wavelengths between 5 and 500 centimeters, when reexamined in the light of physical property data derived from the Apollo program, tentatively support the high heat flows measured in situ and indicate that a regolith thickness between 10 and 30 meters may characterize a large portion of the lunar near side.

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