Orbital velocity is the velocity of celestial body/satellite revolving around another celestial body in circular orbit.
V[tex]
_{o} [/tex] = [tex] \sqrt{ \frac{GM}{R} } [/tex] ---(i)
Escape velocity is the minimum initial velocity a body should be given to escape it from gravitational field.
V[tex] _{escape} [/tex] = [tex] \sqrt{ \frac{2GM}{R} } [/tex] ---- (ii)
Divide (i) and (ii)
[tex] \frac{V_{o} }{V_{escape} } = \frac{1}{ \sqrt{2} } [/tex]
R = radius of circular orbit, M = mass of the celestial body about which satellite/body is performing circular motion. G = Universal gravitational constant