To solve this problem, we will apply principles from fluid mechanics and the physics of motion under gravity.
Step 1: Calculate the terminal velocity of the ball in water
For a sphere moving through a fluid, the terminal velocity \( v_t \) can be calculated using the formula for Stokes' Law:
\(v_t = \frac{2r^2 (\rho - \rho_w)g}{9\eta}\)
Substituting these values into the formula gives:
\(v_t = \frac{2 \times (1 \times 10^{-4})^2 \times (10^5 - 1000) \times 9.8}{9 \times 9.8 \times 10^{-6}}\)
Calculating this yields approximations for simplification:
\(v_t = \frac{2 \times 10^{-8} \times 99000 \times 9.8}{88.2 \times 10^{-6}} \approx 22 \, \text{m/s}\)
Step 2: Use energy conservation to find \( h \)
The ball falls freely under gravity and so its potential energy converts to kinetic energy before entering the water:
\(mgh = \frac{1}{2} mv_t^2\)
Where \( m \) is the mass of the ball, and \( v_t \) is the terminal velocity.
Cancelling \( m \) from both sides gives:
\(gh = \frac{1}{2}v_t^2\)
Hence,
\(h = \frac{v_t^2}{2g}\)
Substitute the known values:
\(h = \frac{22^2}{2 \times 9.8} \approx 2518 \, \text{m}\)
Conclusion: The height \( h \) from which the ball must fall is approximately 2518 m. Therefore, the correct answer is 2518 m.
The terminal velocity \( V_T \) of the spherical ball in water is given by Stokes' law:
\[ V_T = \frac{2gR^2}{9\eta} (\rho_B - \rho_L), \]
where:
Substitute the values into the formula:
\[ V_T = \frac{2 \cdot 9.8 \cdot (1 \times 10^{-4})^2}{9 \cdot 9.8 \times 10^{-6}} (10^5 - 10^3). \]
\[ V_T = \frac{2}{9} \cdot \frac{10 \cdot (10^{-4})^2}{9.8 \times 10^{-6}} \cdot (10^5 - 10^3), \]
\[ V_T = \frac{2}{9} \cdot \frac{10 \cdot 10^{-8}}{9.8 \times 10^{-6}} \cdot (10^5 - 10^3), \]
\[ V_T = \frac{2}{9} \cdot \frac{10}{9.8} \cdot 10^2 = 224.5 \, \text{m/s}. \]
\[ V = \sqrt{2gh}. \]
Rearranging for \( h \):
\[ h = \frac{V^2}{2g}. \]
Substitute \( V_T = 224.5 \, \text{m/s} \) and \( g = 9.8 \, \text{m/s}^2 \):
\[ h = \frac{(224.5)^2}{2 \cdot 9.8}. \]
\[ h = \frac{50402.25}{19.6} \approx 2571 \, \text{m}. \]
Thus, the height \( h \) is approximately:
\[ \boxed{2518 \, \text{m}}. \]
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 : \(A_2 \rightleftharpoons 2A\)