To calculate the acceleration of gravity on the surface of a neutron star with a mass of 3.0x10^30 kg and a radius of 8000 m, the gravitational force equation F = G * m / (d^2) is used, where G is the gravitational constant (6.67x10^-11). The force felt by an object under gravity is proportional to the mass of the star and inversely proportional to the square of the distance from its center. The resulting force calculation yields a value of 3.1265625 x 10^12, which is reasonable for a neutron star despite initial concerns about its magnitude compared to Earth's gravity. It's crucial to ensure all units are consistent, and the calculations confirm that such extreme values are typical for neutron stars. Understanding the relationship between mass, distance, and gravitational force is essential for accurate calculations.