\[ \text{Total energy} = \frac{-GMm}{2(2R)} \] If energy \( \frac{10^4R}{6} \) is added, then \[ \frac{-GMm}{4R} + \frac{10^4R}{6} = \frac{-GMm}{2r} \] where \( r \) is the new radius of revolution and \( g = \frac{GM}{R^2} \). \[ -\frac{mgR}{4} + \frac{10^4R}{6} = -\frac{mgR^2}{2r} \quad (m = 10^3\, \text{kg}) \] \[ -\frac{10^3 \times 10 \times R}{4} + \frac{10^4R}{6} = -\frac{10^3 \times 10 \times R^2}{2r} \] \[ -\frac{1}{4} + \frac{1}{6} = -\frac{R}{2r} \] \[ r = 6R \]
The total mechanical energy of a satellite in a circular orbit is given by:
\[ E = -\frac{GMm}{2r}, \]
where \( G \) is the gravitational constant, \( M \) is the mass of the Earth, \( m \) is the mass of the satellite, and \( r \) is the radius of the orbit.
When energy is supplied to the satellite, the total energy increases, which results in an increase in the radius of the orbit. Let the initial radius of the orbit be \( 2R \), and the new radius be \( r' \).
Using the conservation of energy:
\[ E_{\text{initial}} + \text{Energy supplied} = E_{\text{final}}, \]
\[ -\frac{GMm}{2(2R)} + \frac{10^4R}{6} = -\frac{GMm}{2r'}. \]
Simplifying, we find that the new radius \( r' \) is:
\[ r' = 6R. \]
Thus, the correct answer is \( r' = 6R \), and the correct answer is Option (4).
A black body is at a temperature of 2880 K. The energy of radiation emitted by this body with wavelength between 499 nm and 500 nm is U1, between 999 nm and 1000 nm is U2 and between 1499 nm and 1500 nm is U3. The Wien's constant, b = 2.88×106 nm-K. Then,


What will be the equilibrium constant of the given reaction carried out in a \(5 \,L\) vessel and having equilibrium amounts of \(A_2\) and \(A\) as \(0.5\) mole and \(2 \times 10^{-6}\) mole respectively?
The reaction : \(A_2 \rightleftharpoons 2A\)