$4.2$
Step 1: The nuclear radius is given by the empirical formula: \[ R = R_0 A^{1/3} \] where $A$ is the mass number and $R_0$ is a proportionality constant.
Step 2: Using the ratio of nuclear radii: \[ \frac{R_2}{R_1} = \left( \frac{A_2}{A_1} \right)^{1/3} \] Given $R_1 = 6$ fermi for $A_1 = 125$ and $A_2 = 27$, we compute: \[ R_2 = 6 \times \left( \frac{27}{125} \right)^{1/3} \]
Step 3: Approximating the cube root: \[ \left( \frac{27}{125} \right)^{1/3} = \frac{3}{5} = 0.6 \]
Step 4: \[ R_2 = 6 \times 0.6 = 3.6 { fermi} \]
Step 5: Therefore, the correct answer is (A).
Kepler's second law (law of areas) of planetary motion leads to law of conservation of
Kepler's second law (law of areas) of planetary motion leads to law of conservation of