Distance of the Earth from the Sun, re = 1.5 × 108 km = 1.5×1011 m
Time period of the Earth = Te
Time period of Saturn, Ts = 29. 5 Te
Distance of Saturn from the Sun = rs
From Kepler’s third law of planetary motion, we have
\(T = (\frac{4 \pi^2 r^3 }{ GM})^{\frac{1}{2}}\)
For Saturn and Sun, we can write
\(\frac{rs^3}{ re^3 }= \frac{Ts^2 }{ Te ^2}\)
\(r_s = r_e(\frac{T_s}{ T_e})^{\frac{2}{3}}\)
= 1.5 x 1011 \((\frac{29.5T_e}{T_e})^{\frac{2}{3}}\)
= 1.5 x 1011\( (29.5)^{\frac{2}{3}}\)
= 1.5 x 1011 x 9.55
= 14.32 x 1011 m
Hence, the distance between Saturn and the Sun is 1.432 x 1012 m .
A small point of mass \(m\) is placed at a distance \(2R\) from the center \(O\) of a big uniform solid sphere of mass \(M\) and radius \(R\). The gravitational force on \(m\) due to \(M\) is \(F_1\). A spherical part of radius \(R/3\) is removed from the big sphere as shown in the figure, and the gravitational force on \(m\) due to the remaining part of \(M\) is found to be \(F_2\). The value of the ratio \( F_1 : F_2 \) is:
The height from Earth's surface at which acceleration due to gravity becomes \(\frac{g}{4}\) is \(\_\_\)? (Where \(g\) is the acceleration due to gravity on the surface of the Earth and \(R\) is the radius of the Earth.)
Find the mean and variance for the following frequency distribution.
Classes | 0-10 | 10-20 | 20-30 | 30-40 | 40-50 |
Frequencies | 5 | 8 | 15 | 16 | 6 |
In mechanics, the universal force of attraction acting between all matter is known as Gravity, also called gravitation, . It is the weakest known force in nature.
According to Newton’s law of gravitation, “Every particle in the universe attracts every other particle with a force whose magnitude is,
On combining equations (1) and (2) we get,
F ∝ M1M2/r2
F = G × [M1M2]/r2 . . . . (7)
Or, f(r) = GM1M2/r2
The dimension formula of G is [M-1L3T-2].