Two planets \( A \) and \( B \) have radii \( R \) and \( 1.5R \), and densities \( \rho \) and \( \frac{\rho}{2} \) respectively. The ratio of acceleration due to gravity at the surface of \( B \) to \( A \) is:
Show Hint
For a spherical planet:
\[
g \propto \rho R
\]
- Increasing radius increases gravity.
- Increasing density increases gravity.
- The ratio \( \frac{g_B}{g_A} \) is found using \( g \propto \rho R \).
Step 1: Formula for acceleration due to gravity.
The surface gravity of a planet is given by:
\[
g = \frac{G M}{R^2}
\]
Since mass \( M \) is related to density \( \rho \) and radius \( R \):
\[
M = \rho V = \rho \times \frac{4}{3} \pi R^3
\]
Substituting into the gravity formula:
\[
g = \frac{G (\rho \frac{4}{3} \pi R^3)}{R^2}
\]
\[
g = \frac{4}{3} G \pi \rho R
\]
Thus, gravity at the surface is:
\[
g \propto \rho R
\]
Step 2: Finding the ratio \( \frac{g_B}{g_A} \).
For planet A:
\[
g_A \propto \rho R
\]
For planet B:
- Radius \( R_B = 1.5R \),
- Density \( \rho_B = \frac{\rho}{2} \),
\[
g_B \propto \left(\frac{\rho}{2}\right) (1.5R)
\]
\[
g_B \propto \frac{3}{2} \times \frac{\rho R}{2} = \frac{3}{4} \rho R
\]
Taking the ratio:
\[
\frac{g_B}{g_A} = \frac{\frac{3}{4} \rho R}{\rho R} = \frac{3}{4}
\]
Final Answer:
\[
\boxed{3:4}
\]