The distance of the two planets A and B from the sun are '\(r_A\)' and '\(r_B\)' respectively such that \(r_B = 100\,r_A\). The ratio of the speed of planet A to that of planet B is (both the planets are revolving around the sun)
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For a circular orbit, v = sqrt(GM/r), so v is inversely proportional to the square root of r.