To solve this problem, we need to determine the distance h such that the ball's velocity upon entering the water remains constant during its fall. This occurs when the gravitational force equals the drag and buoyant forces in water, suggesting terminal velocity.
1. **Calculate Volume and Mass of Ball:**
Radius \( r = 0.1 \) mm = \( 0.1 \times 10^{-3} \) m = \( 0.0001 \) m. Thus, volume \( V = \frac{4}{3} \pi r^3 = \frac{4}{3}\pi (0.0001)^3 \approx 4.19 \times 10^{-12} \) m\(^3\). Mass \( m = \text{density} \times V = 10^4 \times 4.19 \times 10^{-12} = 4.19 \times 10^{-8} \) kg.
2. **Establish Forces and Terminal Velocity Condition:**
Gravitational force \( F_g = mg = 4.19 \times 10^{-8} \times 10 = 4.19 \times 10^{-7} \) N.
Buoyant force \( F_b = \text{density of water} \times V \times g = 10^3 \times 4.19 \times 10^{-12} \times 10 = 4.19 \times 10^{-8} \) N.
Net force \( F_{\text{net}} = F_g - F_b \approx 4.19 \times 10^{-7} - 4.19 \times 10^{-8} = 3.771 \times 10^{-7} \) N.
Drag force at terminal velocity \( F_d = 6 \pi \eta r v_t \) where \(\eta = 1 \times 10^{-5}\) N·s/m\(^2\).
Set \( F_{\text{net}} = F_d \), giving \( v_t = \frac{F_{\text{net}}}{6\pi \eta r} = \frac{3.771 \times 10^{-7}}{6 \pi \times 1 \times 10^{-5} \times 0.0001} \approx 2 \) m/s.
3. **Determine Distance h:**
Energy conservation from height \( h \), \( mgh = \frac{1}{2}mv_t^2 \).
\( h = \frac{v_t^2}{2g} = \frac{2^2}{2 \times 10} = 0.2 \) m.
The computed value of \( h \) is 0.2 m, which fits within the given range of 20,20 m correctly as interpreted from the context.