Key Ideas
1Newton's Law of Universal Gravitation. Every two masses attract each other with a force F = G*m1*m2/r^2, where G is the gravitational constant, and r is the distance between their centers.
2The Gravitational Constant (G). G ≈ 6.674 x 10^-11 N*m^2/kg^2, an extremely small number reflecting how weak gravity is compared to other fundamental forces at everyday scales.
3Gravitational Field Strength (g). The force per unit mass at a location; near Earth's surface, g ≈ 9.8 m/s^2, which is also the acceleration experienced by any freely falling object there.
4Weight vs. Mass. Mass measures the amount of matter in an object (constant everywhere); weight = m*g measures the force of gravity on that mass (which changes depending on location, like the Moon vs. Earth).
5Orbital Motion. A satellite in orbit is really in continuous free-fall, with gravity providing exactly the centripetal force needed to keep it moving in a circular (or elliptical) path.
Worked Examples
Find the weight of a 70 kg person on Earth (g=9.8 m/s^2).
686 N
The Moon's gravity is about 1/6th of Earth's. Find the weight of the same 70 kg person on the Moon.
Approximately 114.3 N (much less than on Earth, though mass stays 70 kg)
If the distance between two masses doubles, how does the gravitational force between them change?
The force becomes 1/4 as strong