(c) Escape velocity,
$\mathbf{\ \ \ \ \ \ \ \ \ \ \ \ }v_{ascape}\mathbf{=}\sqrt{\frac{2\ GM}{R}}\mathbf{\ \ }$
$\mathbf{\ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ =}R\sqrt{\frac{8}{3}\pi G\rho}$
$\therefore v_{e} \propto R\ if\ \rho = constant.$
Since the planet is having double radius in comparision to earth, therefore escape velocity becomes twice $ie,$ ${22\ kms}^{- 1}$ .