Use the universal gravitation equation F = G×M×m/r2. Plug in the values of the gravitational constant, the masses and the radius to get F = [6.67408 × 10-11 m3 kg-1 s-2] × [120,000kg] × [400,000kg]/[100m]2. Multiply it out to get F = 6.67408 × 10-11 × 120,000 × 400,000 / (1002) m3 × kg-1 s-2 × kg2 / m2 = 3.20356 × 10-4 kg × m / s2 = 3.20356 × 10-4 N
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