G484 - Circular Motion and Oscillations Flashcards
Degrees to Radians
x (2π/360)
Radians to Degrees
x(360/2π)
State, in terms of force, the conditions necessary for an object to move in a circular path at constant speed
Resultant (centripetal force)
Perpendicular to the direction of motion
Centripetal Acceleration
Directed towards the centre of the circle
Direction of motion is always changing so velocity is always changing even if speed remains constant
Acceleration is the rate of change of velocity
Describe how a mass creates a gravitational field in the space around it
All objects with mass have a gravitational field
The field spreads out into the space around the object in all directions
As a result any other object with mass that is in the field will experience a force of attraction
Gravitational Field Strength
Force per unit mass
Close to the earth’s surface, gravitational field strength is approximately equal to the acceleration of free fall
g = -GM/r²
Newton’s Law of Gravitation
The force between two point masses is proportional to the product of the masses and inversely proportional to the square of the distance between them
F = - GMm/r²
Properties of Gravitational Fields
Unlimited range
Always attractive
Effect all objects with mass
Becomes zero at centre of mass of a sphere as the mass surrounding that point is exerting a force in every direction so the resultant is 0
Period
of an object describing a circle
Time taken for the object to complete one circular path
Kepler’s Third Law
T² ∝ r³
T² = (4π²/GM)r³
Derive T² = (4π²/GM)r³ from first principles
v² = GM/r , v = 2πr/T
(2πr/T)² = GM/r 4π²r²/T² = GM/r 4π²r³ = GMT² T² = (4π²/GM)r³
Geostationary Orbit
24 hour time period
Equatorial orbit - orbits over the equator
Orbits in the same direction as the earth’s rotation
Satellite appears to remain stationary in the sky above a particular point
Radian
The angle subtended by an arc of the circumference equal to the radius
Displacement
Distance form the equilibrium position
Amplitude
Maximum displacement from the equilibrium position
Period
Time taken for one complete oscillation
Frequency
Number of oscillations completed in one second