Two particles of masses m, and m, attract each other gravitationally and are set in motion under the influence of the gravitational force? Will the centre of mass move?
Answer
Since, gravitational force is an internal force, therefore the centre of mass would not move.
Where does a body weigh more at the surface of the earth or in a mine?
Answer
Since value of g in a mine is lesser than at the surface of the Earth, so weight of body in a mine is lesser than the weight of the body on the surface of the earth.
What do you mean by a parking orbit of a satellite?
Answer
The orbit of a satellite which is concentric and coplanar with the equatorial plane of Earth and having a revolution period of 24 hours is called a parking orbit.
The gravitational Potential energy of a body at a point in a gravitational field of another body is $-\frac{\text{GMm}}{\text{r}}$ What does the negative sign show?
Answer
Negative sign means that the mass m is bound to M.
List one difference and one similarity between gravitational and inertial mass.
Answer
Similarity-Both are equal. Difference-Gravitational mass is measured by using comparison of mass by force, but inertial mass measured by the acceleration caused by the force.
The gravitational force between two spheres is x when the distance between their centers is y. What will be the new force if the separation is made 3y?
Answer
Since $\text{F}\propto\frac{1}{\text{r}^2}.$ Therefore, if r is increased by a factor of 3. F will be reduced by a factor of 9. Thus, the new force will be $\frac{\text{x}}{9}.$
Choose the correct alternative: Acceleration due to gravity increases/ decreases with increasing depth (assume the earth to be a sphere of uniform density).
Dimensional formula of ' $\mathrm{g}$ ' $\rightarrow\left[\mathrm{LT}^{-2}\right]$ Dimensional formula of ' $\mathrm{G}$ ' $\rightarrow\left[\mathrm{M}^{-1} \mathrm{~L}^3 \mathrm{~T}^{-2}\right]$
Express the constant $k$ of Eq. $(7.38)$ in days and kilometres. Given $k =10^{-13} s ^2 m ^{-3}$. The moon is at a distance of $3.84 \times 10^5 \ km$ from the earth. Obtain its time-period of revolution in days.
Answer
Given
$k=10^{-13} s ^2 m ^{-3}$
$=10^{-13}\left[\frac{1}{(24 \times 60 \times 60)^2} d ^2\right]\left[\frac{1}{(1 / 1000)^3 \ km ^3}\right]$
$=1.33 \times 10^{-14} d ^2 \ km ^{-3}$
Using Eq. $(7.38)$ and the given value of $k,$ the time period of the moon is
$T^2=\left(1.33 \times 10^{-14}\right)\left(3.84 \times 10^5\right)^3$
$T=27.3 d$
Let the speed of the planet at the perihelion $P$ in Fig. $7.1 (a)$ be $v_p$ and the Sun-planet distance $SP$ be $r_p$ Relate $\left\{r_P, V_P\right\}$ to the corresponding quantities at the aphelion $\left\{r_A, V_A\right\}$. Will the planet take equal times to traverse $\text{B A C}$ and $\text{C P B}$ ?
Answer
The magnitude of the angular momentum at $P$ is $L_p=m_p r_p V_p$, since inspection tells us that $r _p$ and $v _p$ are mutually perpendicular.
Similarly, $L_A=m_p r_A V_A$.
From angular momentum conservation
$m_p r_p V_p=m_p r_A V_A$
$\text { or } \frac{v_p}{v_A}=\frac{r_A}{r_p}$