The Mars atmosphere contains a significant load of suspended dust. Set
tling of atmospheric dust onto the surface of the solar array is poten
tially a lifetime-limiting faster for a power system on any Mars missi
on, For long-term operation of arrays on Mars, it may be necessary to
develop techniques to remove deposited dust, Dust is expected to adher
e to the array by Van der Waals adhesive forces, These forces are quit
e strong at the dust particle sizes expected, If the array surface is
insulating, it is possible that they may also be subject to electrosta
tic adhesion, which may be extremely strong, Dust-removal methods must
overcome this force, Dust-removal methods can be categorized briefly
into four categories: natural, mechanical, electromechanical, and elec
trostatic. The environment of Mars is expected to be an ideal one for
the use of electrostatic dust-removal techniques.