Step 1: Understanding the Concept:
Terminal velocity \( v_t \) is proportional to the square of the radius (\( r^2 \)).
Since mass \( m \propto r^3 \) (for same density), we can relate velocity to mass.
Step 2: Key Formula or Approach:
1. Mass \( m = \frac{4}{3} \pi r^3 \rho \implies r \propto m^{1/3} \).
2. Terminal Velocity \( v_t \propto r^2 \).
3. Combine: \( v_t \propto (m^{1/3})^2 \propto m^{2/3} \).
Step 3: Detailed Explanation:
Let sphere 1 have mass \( m_1 = 8 \) g and velocity \( v_1 = 3 \) cm/s.
Let sphere 2 have mass \( m_2 = 64 \) g and velocity \( v_2 \).
Ratio:
\[ \frac{v_2}{v_1} = \left( \frac{m_2}{m_1} \right)^{2/3} \]
Substitute values:
\[ \frac{v_2}{3} = \left( \frac{64}{8} \right)^{2/3} \]
\[ \frac{v_2}{3} = (8)^{2/3} = (2^3)^{2/3} = 2^2 = 4 \]
\[ v_2 = 3 \times 4 = 12 \, \text{cm/s} \]
Step 4: Final Answer:
The terminal velocity is \( 12 \, \text{cms}^{-1} \).