This document provides information about acceleration due to gravity. It defines acceleration due to gravity as the acceleration of a freely falling body due to the gravitational force of attraction exerted by the Earth. It is denoted by 'g' and is independent of the mass of the falling body. The value of 'g' depends on the distance from the center of the Earth and varies from 9.83 m/s^2 at the poles to 9.79 m/s^2 at the equator. 'g' decreases with increasing distance from the Earth's surface and is zero at the Earth's center. The value of 'g' also varies for other planets depending on their radius and mass.