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Let the period of revolution of a planet at a distance R from a star be T. Prove that if it was at a distance of 2R from the star, its period of revolation will be sqrt8T. |
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Answer» Solution :`T= (2PI)/(SQRT(GM)) r^(3//2), ` where T = period of revolution of a planet around the sun, M= mass of the sun, G = GRAVITATIONAL constant and r = radius of the orbit assumed to be circular = distance of the planet from the sun. For` r= R and T = T_(1)` ` T_(1) = (2pi)/(sqrt(GM)) R^(3//2)` From r = 2 R and T = `T_(2)` ` T_(2) = (2pi)/(sqrt(GM)) (2R)^(3//2) = (2pi)/(sqrt(GM)) R^(3//2) xx 2^(3//2)= T_(1) xx 2^(3//2)` ` T_(2) = T_(1) sqrt(8) = sqrt(8)T` |
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