01 Key Concepts
Newton'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.
The Gravitational Constant (G)
G โ 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.
Gravitational Field Strength (g)
The force per unit mass at a location; near Earth's surface, g โ 9.8 m/s^2, which is also the acceleration experienced by any freely falling object there.
Weight 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).
Orbital 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.
02 Key Formulas
- F = G*m1*m2/r^2
- Weight = m*g
03 Solved Examples
- Apply Weight = m*g = 70*9.8.
- Moon's g โ 9.8/6 โ 1.63 m/s^2.
- Weight = 70*1.63.
- Force is inversely proportional to r^2 (the square of distance).
- Doubling r means dividing force by 2^2 = 4.
04 Practice Questions
๐ Gravitation โ Downloadable Worksheet
10 questions with a full answer key. Grab the PDF to print, or try the interactive version in your browser.