Related Questions

    3.

    The radius of the earth is 6400 km6400 \mathrm{~km} and g=10 m/sec2g=10 \mathrm{~m} / \mathrm{sec}^2. In order that a body of 5 kg5 \mathrm{~kg} weighs zero at the equator, the angular speed of the earth is

    A

    1/80radian/sec1 / 80 \,\mathrm{radian} / \mathrm{sec}

    B

    1/400radian/sec1 / 400 \,\mathrm{radian} / \mathrm{sec}

    C

    1/800radian/sec1 / 800 \,\mathrm{radian} / \mathrm{sec}

    D

    1/1600radian/sec1 / 1600 \,\mathrm{radian} / \mathrm{sec}

    Question Tags

    5.

    The earth moves round the sun in a near circular orbit of radius 1.5imes10111.5 imes {10^{11}} m. Its centripetal acceleration is

    A

    1.5imes103  m/s21.5 imes {10^{ - 3}}\;m/{s^2}

    B

    3imes103  m/s23 imes {10^{ - 3}}\;m/{s^2}

    C

    6imes103  m/s26 imes {10^{ - 3}}\;m/{s^2}

    D

    12imes103  m/s212 imes {10^{ - 3}}\;m/{s^2}

    Question Tags

    6.

    Which of the following statements is true about 'G'?

    A

    It is a fundamental constant.

    B

    Its value depends on the medium between the objects.

    C

    Its value is different on different planets.

    D

    It has the units of force.

    Question Tags

    7.

    The planets with radii R1R_1 and R2R_2 have densities ρ1\rho_1 and ρ2\rho_2, respectively. Their atmospheric pressures are p1p_1 and p2p_2, respectively. Therefore, the ratio of masses of their atmospheres, neglecting variation of gg within the limits of atmosphere is

    A

    ρ1R2p1/ρ2R1p2\rho_1 R_2 p_1 / \rho_2 R_1 p_2

    B

    p1R2ρ2/pP2R1ρ1p_1 R_2 \rho_2 / p P_2 R_1 \rho_1

    C

    p1R1ρ1/p2R2ρ2p_1 R_1 \rho_1 / p_2 R_2 \rho_2

    D

    p1R1ρ2/p2R2ρ1p_1 R_1 \rho_2 / p_2 R_2 \rho_1

    Question Tags

    company logo