G484 Definitions Flashcards
Essential definitions and physical laws you must be able to remember for the G484 Unit
Newton’s 1st Law
An object will remain at rest or keep travelling at a constant velocity unless it is acted on by an external force.
Newton’s 2nd Law
The net force acting on an object is equal to the rate of change of momentum. The net force and the change in momentum are in the same direction.
Newton’s 3rd Law
When two bodies interact they exert equal and opposite forces of the same kind on each other.
Linear Momentum
The product of an objects mass and its velocity.
Net Force
The resultant of all the forces acting on an object.
Impulse of a Force
The product of a force and the time for which it acts.
Conservation of Momentum
In a closed system, when bodies interact, the total momentum in any specified direction remains the same.
Perfectly Elastic Collision
A collision in which kinetic energy is conserved (momentum and total energy always conserved).
Inelastic Collision
A collision in which kinetic energy is not conserved (momentum and total energy are conserved).
Radian
The angle subtended at the centre of a circle when the arc length is equal to the radius. Pi radians equals 180 degrees.
Gravitational Field Strength
The gravitational force per unit mass.
Newton’s Law of Gravitation
Any two point masses attract each other with a force that is directly proportional to the product of their masses and inversely proportional to the square of their separation.
Period
The time taken by an object to complete one orbit or for one complete oscillation by a vibrating object.
Geostationary Orbit
The orbit of a satellite which has a period of one day and is in the equatorial plane.
Simple Harmonic Motion
Motion of an oscillator where acceleration is directly proportional to the displacement and is directed towards the equilibrium position.