Two planets are revolving around a star in circular orbits. If the ratio of radii of orbit is 1:4, then ratio of their time period is
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we know, T^2 proportional to R^3.... so T1 : T2 = (R1 : R2)^(3/2)......so T1 : T2 = 1 : 8.....using Galileos laws of planetary motion
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