Unit 4- Gravity, Orbits, Circular Motion and Simple Harmonic motion Flashcards
Newton’s law of Gravitation
The gravitational force between two masses is proportional to the product of the masses and inversely proportional to the square of the distance between them
Keepler’s third law
The cube of the planets distance from the Sun divided by the square of the orbital period is the same for all planets
Conditions for circular motion
Resultant force acts perpendicular to the velocity
Geostationary orbit
An equatorial orbit with a period equal to the rotation period of the earth and in the same direction
Radian
2 Pi radians = 360 degrees
Simple Harmonic motion
- Acceleration is proportional to displacement
2. Acceleration is directed in the opposite direction to the displacement
Displacement (in SHM)
Distance of a body from its equilibrium position
Amplitude
Maximum displacement
Gravitational field strength
Force per unit mass at a point in a gravitational field
Frequency
Number of oscillation per second
Angular frequency
2Pi x frequency or 2Pi/T
Phase difference
An angular measure of how much one oscillation leads or lags another oscillation
Resonance
When the frequency of oscillation of the driving force is very close to the natural frequency of the driven system. Resulting is maximum energy transfer to the driven system, leading to very large amplitude oscillation