The potential is described of a candidate Mars Observer altimeter for determining dielectric properties of Mars regolith. It is pointed out that it is straightforward to use the time between altimeter pulse trains for passive radiometry (hence dielectric properties) and roughness can be derived. Given the mission plan the whole surface can be mapped at least three times, yielding data on seasonal variability.
Tilman Spohn, T. L. Hudson, Eloïse Marteau, M. Golombek, M. Grott, Torben Wippermann, Kausar Ali, Cédric Schmelzbach, S. Kedar, K. Hurst, A. Trebi‐Ollennu, V. Ansan, James Jim Brian Garvin, J. Knollenberg, Nils Mueller, S. Piqeux, Roy Lichtenheldt, C. Krause, Cinzia Fantinati, Nienke Brinkman, David Sollberger, Pierre Delage, Christos Vrettos,
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