Step 1: Write the formula for escape velocity.
Escape velocity from a planet is
\[
v_e=\sqrt{\frac{2GM}{R}}.
\]
For a spherical planet,
\[
M=\frac{4}{3}\pi R^3\rho.
\]
Substituting this in the formula,
\[
v_e=\sqrt{\frac{2G}{R}\cdot \frac{4}{3}\pi R^3\rho}
\]
\[
v_e=\sqrt{\frac{8}{3}\pi G\rho R^2}
\]
Therefore,
\[
v_e\propto R\sqrt{\rho}.
\]
Step 2: Compare escape velocities of the two planets.
Let the original planet have radius \(R\) and density \(\rho\).
The new planet has radius
\[
R'=3R
\]
and density
\[
\rho'=2\rho.
\]
Therefore,
\[
\frac{v'_e}{v_e}
=
\frac{R'\sqrt{\rho'}}{R\sqrt{\rho}}
\]
\[
=
\frac{3R\sqrt{2\rho}}{R\sqrt{\rho}}
\]
\[
=3\sqrt{2}.
\]
Step 3: Find the escape velocity from the second planet.
Given,
\[
v_e=16\,\text{km s}^{-1}.
\]
Thus,
\[
v'_e=3\sqrt2\times 16
\]
\[
v'_e=48\sqrt2\,\text{km s}^{-1}.
\]
Comparing with
\[
V\sqrt2,
\]
we get
\[
V=48.
\]
Step 4: Final conclusion.
Therefore,
\[
\boxed{48}
\]