Chapter 11 Flashcards
What is Newton’s first law of motion?
Any object remains in a state of uniform motion unless a resultant external force acts on it
What is Newton’s second law of motion?
The acceleration of an object is proportional to the resultant force upon it. Force is proportional to the rate of change of momentum.
What is Newton’s third law of motion?
If body A exerts a force on body B, then body B exerts a force of the same magnitude but the opposite direction and the same type on body A
How do you calculate momentum?
p=m*v units are kg m s^-1
What are the 2 most important things to remember about momentum?
It is conserved in a closed system
It is a vector quantity
How do you calculate the change in momentum?
Final momentum - Initial momentum
What is impulse?
The change in momentum
What are the 2 equations for calculating impulse?
Final momentum - initial momentum
Average force * time applied for
What are the 3 categories of collisions, and how do they differ?
1) they coalesce: totally inelastic collision
2) Elastic collision: kinetic energy is conserved
3) Inelastic collision: some kinetic energy is lost, but they do ‘bounce’
What is the full equation associated with Newton’s second law of motion?
F=m(dv/dt) + v(dm/dt)
But dm/dt is nearly always 0, so can be simplified to F=ma in most cases
What is Kepler’s first law?
A planet moves in an ellipse with the Sun at one focus
What is Kepler’s second law?
The line from the Sun to a planet sweeps out equal areas in equal times
What is Kepler’s third law?
Square of orbital time is proportional to cube of orbital radius
How do you calculate acceleration towards the centre of a circle?
a=v^2/r
How do you calculate centripetal force?
F=mv^2/r =m(omega)^2 r