Finally, calculating gravitational acceleration becomes especially important when you’re dealing with planets or celestial bodies other than Earth. Use Newton’s Law of Universal Gravitation:
g = G * (M / r²)
In this formula:
- G represents the gravitational constant
- M is the mass of the celestial body
- r is the distance from its center to the object
This allows you to calculate gravity on the Moon, Mars, or any celestial body.