\(\frac{v}{4}\)
To solve this problem, we need to understand the concept of terminal velocity in a viscous medium according to Stokes' Law. The terminal velocity \( v_t \) for a spherical object of radius \( r \) and density \( \rho \) falling through a medium with viscosity \( \eta \) is given by:
\(v_t = \frac{2}{9} \cdot \frac{r^2 (\rho - \rho_m)}{\eta} \cdot g\)
where:
For the first ball with radius \( r \), the terminal velocity is \( v \).
For the second ball with the same mass but a radius of \( 2r \), let's consider the terminal velocity \( v_2 \).
The mass of the sphere is proportional to the volume, which is proportional to \( r^3 \). Hence, keeping the mass constant implies:
\(\rho \cdot r^3 = \rho_2 \cdot (2r)^3\)
The density of the new sphere \( \rho_2\) will be:
\(\rho_2 = \frac{\rho}{8}\)
Now applying these changes to the terminal velocity formula for the second ball:
\(v_2 = \frac{2}{9} \cdot \frac{(2r)^2 (\rho_2 - \rho_m)}{\eta} \cdot g\)
Substitute \(\rho_2 = \frac{\rho}{8}\):
\(v_2 = \frac{2}{9} \cdot \frac{4r^2 \left(\frac{\rho}{8} - \rho_m\right)}{\eta} \cdot g\)
Thus:
\(v_2 = \frac{2}{9} \cdot \frac{r^2 (\rho - \rho_m)}{\eta} \cdot \frac{1}{2} \cdot g = \frac{v}{2}\)
Substituting the known relationship we find:
The terminal velocity for the second ball is \( \frac{v}{2} \).
Hence, the correct answer is \(\frac{v}{2}\).
Since the density of the medium is negligible, the buoyancy force can be ignored. At terminal velocity, the gravitational force on the ball is balanced by the viscous drag force. The terminal velocity \( v \) is given by:
\[ v \propto \frac{1}{r}, \]for a sphere of constant mass.
Let the terminal velocity of the original ball (radius \( r \)) be \( v \) and the terminal velocity of the larger ball (radius \( 2r \)) be \( v' \).
Using the inverse proportionality:
\[ \frac{v}{v'} = \frac{r'}{r}. \]Since \( r' = 2r \):
\[ \frac{v}{v'} = 2 \implies v' = \frac{v}{2}. \]Thus, the terminal velocity of the larger ball is:
\[ \frac{v}{2}. \]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 : \(A_2 \rightleftharpoons 2A\)