The acceleration due to gravity is given by,
g=GMR2g =G\frac{M}{R^2}g=GMR2
MMM the mass of the planet and
RRR is the distance of the point under consideration from the centre of the planet.
(i) due to height above or below the surface of planet,
g′=g(1+hR)−2,wherehisheightabovethesurfaceoftheplanet
g′=g(1−hR),wherehisdepthbelowthesurfaceoftheplanet
(ii) Due to shape of planet, as it bulges out of the equator and flat on poles.
Re>Rp≅21km
∴gp>ge
(iii) Due to rotation of the planet
g′=gp−rω2cos2λ
Therefore, acceleration due to gravity (ggg) depends on the mass of the planet, distance between centre of planet and object, shape of the planet, rotational parameters of the planet.