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    8.

    The acceleration due to gravity at height hh above the earth if h<<Rh < < R (Radius of earth) is given by

    A

    gβ€²=g(1βˆ’h22R2)g^{\prime}=g\left(1-\frac{h^{2}}{2 R^{2}}\right)

    B

    gβ€²=g(1βˆ’h2R)g^{\prime}=g\left(1-\frac{h}{2 R}\right)

    C

    gβ€²=g(1βˆ’2hR)g^{\prime}=g\left(1-\frac{2 h}{R}\right)

    D

    gβ€²=g(1βˆ’2h2R2)g^{\prime}=g\left(1-\frac{2 h^{2}}{R^{2}}\right)

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    10.

    Two planets of mean distance d1 and d2{d_1}\,and\,{d_2} from the sun and their frequencies are n1 and n2{n_1}\,and\,{n_2} respectively then

    A

    n12d12=n2d22n_1^2d_1^2 = {n_2}d_2^2

    B

    n22d23=n12d13n_2^2d_2^3 = n_1^2d_1^3

    C

    n1d12=n2d22{n_1}d_1^2 = {n_2}d_2^2

    D

    n12d1=n22d2n_1^2{d_1} = n_2^2{d_2}

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