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.
Figures 9.20(a) and (b) refer to the steady flow of a (non-viscous) liquid. Which of the two figures is incorrect ? Why ?
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]