A charge of 32 `microC, located at the origin, is attached to a large mass and can be considered stationary. A charge of -44.01 `microC is attached to a relatively small mass of .0032 kg. The second charge orbits the first in a circular orbit which passes through ( .42 m, 0, 0). What is its orbital velocity?
The key here is that the Coulomb force of attraction must provide the centripetal force which results in the centripetal acceleration v^2/r of the orbiting mass.
An orbit of radius r and velocity v requires a centripetal acceleration of a = v^2 / r. If the orbiting mass is m, then the corresponding centripetal force required to maintain the circular path is F = ma = m v^2 / r. In this case the centripetal force is supplied by the Coulomb attraction | F | = k | q1 | | q2 | / r^2 . Thus we have
m v^2 / r = k | q1 | | q2 | / r^2.
We easily solve this equation for v to obtain
v = `sqrt( k | q1 q2 | / (m r) ).
The figure below shows the Coulomb force F on the orbiting charge. The circular orbit bounds the shaded circle. The centripetal acceleration a is directed toward the center of the circle, where the fixed charge q1 resides.
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