\(\frac{3π }{5}\)
\(\frac{π }{6}\)
\(\frac{6π }{5}\)
\(\frac{5π }{6}\)
To solve this problem, we need to determine the height \(h_Q\) of satellite Q above the Earth's surface. Given:
\(h_P = \frac{R}{3}\)
\(\frac{g_P}{g_Q} = \frac{36}{25}\)
We know that the gravitational acceleration \(g\) at a height \(h\) is given by:
\(g = \frac{g_0}{(1+\frac{h}{R})^2}\)
where \(g_0\) is the gravitational acceleration at the Earth's surface. For satellite P:
\(g_P = \frac{g_0}{(1+\frac{h_P}{R})^2}\)
\(g_P = \frac{g_0}{(1+\frac{R}{3R})^2} = \frac{g_0}{(\frac{4}{3})^2} = \frac{9g_0}{16}\)
For satellite Q:
\(g_Q = \frac{g_0}{(1+\frac{h_Q}{R})^2}\)
Using the relationship \(\frac{g_P}{g_Q} = \frac{36}{25}\), we get:
\(\frac{\frac{9g_0}{16}}{\frac{g_0}{(1+\frac{h_Q}{R})^2}} = \frac{36}{25}\)
This can be simplified to:
\(\frac{9}{16} \times (1+\frac{h_Q}{R})^2 = \frac{36}{25}\)
On further simplification,
\((1+\frac{h_Q}{R})^2 = \frac{16}{9} \times \frac{36}{25} = \frac{64}{25}\)
Taking the square root:
\(1+\frac{h_Q}{R} = \frac{8}{5}\)
\(\frac{h_Q}{R} = \frac{8}{5} - 1 = \frac{3}{5}\)
Hence:
\(h_Q = \frac{3R}{5}\)
The correct answer is therefore:
\(\frac{3R}{5}\)
Given \(h_p=\frac{R}{3}\)
\(h_q=?\)
gravitational acceleration at height
\(g_{ht}=\frac{GM}{(R+h)^2}\)
\(\frac{g_P}{g_Q}=\frac{36}{25}\)
\(=\frac{\frac{GM}{(R+h_p)^2}}{\frac{GM}{(R+h_Q)^2}}\)
when \(h_P=\frac{R}{3}\)
on solving we get
\(h_Q=\frac{3R}{5}\)
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: 
Match the LIST-I with LIST-II
\[ \begin{array}{|l|l|} \hline \text{LIST-I} & \text{LIST-II} \\ \hline \text{A. Gravitational constant} & \text{I. } [LT^{-2}] \\ \hline \text{B. Gravitational potential energy} & \text{II. } [L^2T^{-2}] \\ \hline \text{C. Gravitational potential} & \text{III. } [ML^2T^{-2}] \\ \hline \text{D. Acceleration due to gravity} & \text{IV. } [M^{-1}L^3T^{-2}] \\ \hline \end{array} \]
Choose the correct answer from the options given below:
The center of a disk of radius $ r $ and mass $ m $ is attached to a spring of spring constant $ k $, inside a ring of radius $ R>r $ as shown in the figure. The other end of the spring is attached on the periphery of the ring. Both the ring and the disk are in the same vertical plane. The disk can only roll along the inside periphery of the ring, without slipping. The spring can only be stretched or compressed along the periphery of the ring, following Hookeβs law. In equilibrium, the disk is at the bottom of the ring. Assuming small displacement of the disc, the time period of oscillation of center of mass of the disk is written as $ T = \frac{2\pi}{\omega} $. The correct expression for $ \omega $ is ( $ g $ is the acceleration due to gravity): 
Let $ a_0, a_1, ..., a_{23} $ be real numbers such that $$ \left(1 + \frac{2}{5}x \right)^{23} = \sum_{i=0}^{23} a_i x^i $$ for every real number $ x $. Let $ a_r $ be the largest among the numbers $ a_j $ for $ 0 \leq j \leq 23 $. Then the value of $ r $ is ________.
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 Newtonβs law of gravitation, βEvery particle in the universe attracts every other particle with a force whose magnitude is,
On combining equations (1) and (2) we get,
F β M1M2/r2
F = G Γ [M1M2]/r2 . . . . (7)
Or, f(r) = GM1M2/r2
The dimension formula of G is [M-1L3T-2].