Step 1: Use surface area of sphere.
\[
A = 4\pi R^2
\]
Step 2: Compare radii of planets \( P \) and \( Q \).
Since surface areas are \( A \) and \( 4A \), radius of \( Q \) is twice radius of \( P \):
\[
R_Q = 2R_P
\]
Step 3: Use mass-density relation.
For same density:
\[
M \propto R^3
\]
Step 4: Compare masses.
\[
M_Q = 8M_P
\]
Step 5: Find mass of planet \( R \).
\[
M_R = M_P + M_Q
\]
\[
M_R = M_P + 8M_P = 9M_P
\]
Step 6: Relate escape velocity with radius.
Escape velocity is:
\[
V = \sqrt{\frac{2GM}{R}}
\]
For same density, \( M \propto R^3 \), so:
\[
V \propto R
\]
Step 7: Compare escape velocities.
\[
R_Q = 2R_P
\]
\[
R_R = \sqrt[3]{9}R_P
\]
Since \( \sqrt[3]{9} > 2 \), therefore:
\[
V_R > V_Q > V_P
\]