The physical properties, surface morphology, crater ejecta, and origin of Mars' moons Phobos and Deimos are considered in light of the intensive research done through the Mariner and Viking missions. Particular attention is given to orbits, secular acceleration and tides, photometric properties and phase curves, crater densities, grooves on Phobos, cratering mechanics, and dust belts.
The moons of Mars
1980-01-01
Miscellaneous
No indication
English
Online Contents | 2006
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