The equation for calculating the gravitational field strength of a single body is expressed as GM/r, where G is the gravitational constant, M is the mass of the body, and r is the distance from the center. Gravity is indeed stronger closer to the center of a massive body, but as one approaches the center of the Earth, the gravitational force decreases to zero. This decrease in gravity is due to the assumption in Newtonian gravity that all mass is concentrated at the center, which only holds true outside the body. For a uniform spherical mass distribution, specific equations apply for regions inside and outside the body. Understanding these principles is crucial for accurately calculating gravitational effects.