<Dl> <Dd> g h = g 0 (r e r e + h) 2 (\ displaystyle g_ (h) = g_ (0) \ left ((\ frac (r_ (\ mathrm (e))) (r_ (\ mathrm (e)) + h)) \ right) ^ (2)) </Dd> </Dl> <Dd> g h = g 0 (r e r e + h) 2 (\ displaystyle g_ (h) = g_ (0) \ left ((\ frac (r_ (\ mathrm (e))) (r_ (\ mathrm (e)) + h)) \ right) ^ (2)) </Dd> <Ul> <Li> g is the gravitational acceleration at height h above sea level . </Li> <Li> r is the Earth's mean radius . </Li> <Li> g is the standard gravitational acceleration . </Li> </Ul> <Li> g is the gravitational acceleration at height h above sea level . </Li>

Variation of g due to altitude latitude and depth