Concept:
Escape velocity is the minimum velocity required for an object to escape the gravitational field of a planet without returning.
\[
v_e = \sqrt{\frac{2GM}{R}}
\]
Orbital velocity is the velocity required for a satellite to remain in circular orbit around a planet.
\[
v_o = \sqrt{\frac{GM}{R}}
\]
where
\(G\) = gravitational constant,
\(M\) = mass of the planet,
\(R\) = radius of the planet.
Step 1: Write the ratio of escape velocity to orbital velocity.
\[
\frac{v_e}{v_o}
=
\frac{\sqrt{\frac{2GM}{R}}}{\sqrt{\frac{GM}{R}}}
\]
Step 2: Simplify the expression.
\[
\frac{v_e}{v_o} = \sqrt{2}
\]
Thus the ratio is
\[
\sqrt{2} : 1
\]