SUBSURFACE EMISSIONS FROM MERCURY - VLA RADIO OBSERVATIONS AT 2 AND 6 CENTIMETERS

We present radio observations of Mercury made with the VLA; once in 1986, and on two dates in February of 1988. These observations are the first to spatially map both hot regions associated with the theoretical "hot poles." These "hot poles" are separated by 180-degrees and are a result of the unusual diurnal heating from Mercury's 3/2 spin-orbit resonance and eccentric orbit. Our highest resolution data maps areas of the planet as small as 330 km. We include maps of total intensity, brightness temperature, polarized intensity, fractional polarization, depolarization, and spectral index. We find that the subsurface thermal emissions from Mercury are characteristic of blackbody reradiation from the solar insolation over a diurnal cycle. We use these observations to produce full-disk thermophysical models. We have solved the one-dimensional, time-dependent heat-diffusion equation for all observed disk elements at each epoch in order to constrain thermophysical parameters and properties of the subsurface material. Using typical lunar values for several of the parameters, we are able to reproduce the temperature morphology and most of the observed temperature values. We do, however, find that the best-fit models require a substantial contribution of the heat transport in the subsurface to be radiative in nature. The primary difficulty in our models is in predicting the observed temperature differences as a function of frequency.