If the gravitational force between two objects were proportional to $\frac{1}{R}$ (and not as $\frac{1}{R^2}$), where R is the distance between them, then a particle in a circular path (under such a force) would have its orbital speed v, proportional to:
(1994, 89)
1. $R$
2. $R^0$ (independent of R)
3. $\frac{1}{R^2}$
4. $\frac{1}{R}$
View Answer
Centripetal force is provided by the given gravitational force: $$\frac{mv^2}{R} = \frac{k}{R}$$.
Solving for $v$, we get $v^2 = \frac{k}{m}$.nSince $k$ and $m$ are constants, $v$ is independent of $R$, meaning $v \propto R^0$.
The mean radius of earth is R, its angular speed on its own axis is $\omega$ and the acceleration due to gravity at earth’s surface is g. What will be the radius of the orbit of a geostationary satellite?
(1992)
1. $(\frac{R^2g}{\omega^2})^{\frac{1}{3}}$
2. $(\frac{Rg}{\omega^2})^{\frac{1}{3}}$
3. $(\frac{R^2\omega^2}{g})^{\frac{1}{3}}$
4. $(\frac{R^2g}{\omega})^{\frac{1}{3}}$
View Answer
Gravitational force provides the centripetal force: $$\frac{GMm}{r^2} = m\omega^2r$$.nSince $$g = \frac{GM}{R^2}$$, we can write $$GM = gR^2$$.nSubstituting this gives $$\frac{gR^2}{r^2} = \omega^2r \Rightarrow r^3 = \frac{gR^2}{\omega^2} \Rightarrow r = (\frac{R^2g}{\omega^2})^{\frac{1}{3}}$$.