In this case, if you equal the centripetal force to the force due to the magnitude of the gravitational field, you obtain:
[tex]\frac{1}{2}m\frac{v^2}{R}=mg^{\prime}[/tex]By solving for v into the previous equation, you get:
[tex]v=\sqrt[]{2Rg^{\prime}}[/tex]where,
R: radius of the planet = 6.00*10^7 m
g; gravitational acceleration constant = 46.0 m/s^2
v: escape speed.
Replace the values of the parameters into the formula for v:
[tex]\begin{gathered} v=\sqrt[]{2(6.00\cdot10^7m)(46.0\frac{m}{s^2})} \\ v\approx74,296.7\frac{m}{s} \end{gathered}[/tex]Hence, the escape speed is approximately 74,296.7 m/s