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Physics test 2

TermDefinition
force a push or pull on an object
mass a measure of how much inertia an object has
Newton's 1st Law every object continues in its state of rest, or of uniform velocity in a straight line, as long as no net force acts on it
Newton's 2nd Law F = ma
Newton's 3rd Law If object A exerts a force on object B, then object B exerts a force of the same magnitude on object A but in the opposite direction
weight the force on an object due to gravity
kinetic frictional force F(fr) = u(k)*F(N)
maximum static frictional force F(fr) is less than or equal to u(s)*F(N)
centripetal acceleration a(rad) = (v^2)/r
direction of centripetal acceleration towards the center of the circle
period (T) the time it takes to complete one revolution
speed in terms of the period v = (2*pi*r)/T
a(rad) in terms of the period a = (4*pi*r^2)/T^2
centripetal acceleration net force F = (m*v^2)/r
universal constant G 6.67*10^-11
force of gravity G (m1*m2)/r^2
period of an orbit T^2 = ((4*pi^2)/(G*m(E))) * r^3
work F*d*cos(theta)
joule (J) the SI unit for work
kinetic energy 1/2*m*v^2
work energy theorem W(net) = delta KE
potential energy in terms of work W = -delta PE
work done by gravity on a falling object -m*g*(y2-y1)
potential energy mgy
Hooke's Law F(ext) = k*x
elastic potential energy 1/2*k*x^2
conservative force work done is independent of the path followed
non-conservative force work done depends on the path taken
zero-work forces never do any work
power W/delta t
watt (W) the SI unit for power
power for a constant force p = F*v*cos(theta)
momentum p = m*v
Kg*m/s the SI unit for momentum
isolated system the total force on the system is zero, momentum is conserved
impulse F* delta t
N*s the SI unit for impulse
impulse-momentum theorem F = delta p/delta t
elastic collision a collision where both the total kinetic energy and momentum are conserved
inelastic collision a collision where momentum is conserved but total kinetic energy is not
Created by: imr36093
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