Lesser by a factor of 0.63
Time taken by the Earth to complete one revolution around the Sun, Te = 1 year
Orbital radius of the Earth in its orbit, Re = 1 AU
Time taken by the planet to complete one revolution around the Sun, \(T_p = \frac{1}{2} T_e = \frac{1}{2}\) year
Orbital radius of the planet = Rp
From Kepler’s third law of planetary motion, we can write:
\((\frac{R_p}{R_e})^3 = (\frac{T_p }{ T_e})^2\)
\(\frac{R_p}{R_e} = (\frac{T_p}{T_e})^{\frac{2}{3}}\)
\(=(\frac{\frac{1}{2}}{1} )^{\frac{2}{3}}= (0.5)^{\frac{2}{3} }= 0.63\)
Hence, the orbital radius of the planet will be 0.63 times smaller than that of the Earth.
Net gravitational force at the center of a square is found to be \( F_1 \) when four particles having masses \( M, 2M, 3M \) and \( 4M \) are placed at the four corners of the square as shown in figure, and it is \( F_2 \) when the positions of \( 3M \) and \( 4M \) are interchanged. The ratio \( \dfrac{F_1}{F_2} = \dfrac{\alpha}{\sqrt{5}} \). The value of \( \alpha \) is 

Find the mean deviation about the mean for the data 38, 70, 48, 40, 42, 55, 63, 46, 54, 44.
Gravitational force is a central force that depends only on the position of the test mass from the source mass and always acts along the line joining the centers of the two masses.
According to Newton’s law of gravitation, “Every particle in the universe attracts every other particle with a force whose magnitude is,
By combining equations (1) and (2) we get,
F ∝ M1M2/r2
F = G × [M1M2]/r2 . . . . (7)
Or, f(r) = GM1M2/r2 [f(r)is a variable, Non-contact, and conservative force]