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Surface evolution on the Martian satellites under the influence of Mars
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A thermal model of the Martian satellites
Icarus, 1989Abstract A thermal model of the Martian satellites is developed that takes into account their ellipsoidal shape, eclipse effects, the temperature dependence of the heat conduction coefficient, and the reflected and thermal radiation of Mars. Results for the diurnal temperature behavior of Phobos and Deimos for different latitudes, longitudes, and ...
Ekkehard Kuhrt
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Photometric properties of the Martian satellites
Icarus, 1974New photoelectric observations yield V(1, alpha) equals 12.95 + 0.036 alpha + or - 0.05, B-V equals 0.65 + or - 0.03, and U-B equals 0.18 + or - 0.03 for Deimos and V(1, 0) equals 11.9 + or - 0.2 for Phobos. The derived geometric albedos of both satellites are near 0.065.
B.H. Zellner, R.C. Capen
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