`F = (GMm)/r^2`where,F − gravitational forceG − gravitational constantM − mass of the earthm − mass of object
r − distance
(i). r = doubled`F = (GMm)/r^2` keeping everything constant i.e. G, M, m= `(GMm)/(2r)^2`= `(GMm)/(4r^2)`
F becomes one-fourth.
(ii) r = halved`F = (GMm)/r^2` keeping everything constant i.e. G, M, m= `(GMm)/(1/(2r))^2`= `(GMm)/(1/(4r))^2`= `(4GM m)/(r^2)`
F becomes four times the original.