The correct option is B Gravitational Potential Energy
Gravitational PE of the satellite about the planet is: U=−GMpmsr here the subscripts p and s refer to the planet and satellite respectively.
As the satellite moves to an orbit of greater radius, PE becomes less negative, hence it increases.
Gravitational force is ∝1r2, hence it decreases when r increases.
Centripetal acceleration is due to gravitational force, hence it also decreases.
Angular momentum: L=mvr is conserved. where v is the linear speed.
As r increases, v decreases.