According to Newton's Law of Universal Gravitation, the gravitational force (F) between two objects with masses M₁ and M₂ is directly proportional to the product of their masses and inversely proportional to the square of the distance (r) between their centers: F = G (M₁ M₂) / r². In this case, M₁ is the mass of the Earth (M_earth) and M₂ is the mass of the Moon (M_moon). Let the original distance be r. The original gravitational force is F = G (M_earth M_moon) / r². If the distance is halved, the new distance is r' = r/2. The new gravitational force F' will be: F' = G (M_earth M_moon) / (r')² F' = G (M_earth M_moon) / (r/2)² F' = G (M_earth M_moon) / (r²/4) F' = 4 [G (M_earth M_moon) / r²] So, F' = 4 F. The gravitational force increases to four times its original value.