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Center of mass of a system of two particles:
Xcm = (x1m1+x2m2)/(m1+m2)
Center of mass of a group of particles
Xcm = sum(mr)/sum(m)
Cener of mass beyond a linear sysem
solve in component form
Momentum formula
p = mv, delt p = m delt v, p = Ft (If force does not change)
Newton’s second law in terms of momentum
sum(F) = dp/dt.
Impulse
The change in momentum, J = dp = int(F)dt
Law of conservation of momentum
Momentum never changes, if KE is conserved elastic, if KE not conserved inelastic, perfectly inelastic means objects stick together afterwards.
How to calculae theta in uniform circular motion
theta = distance traveled on perimeter / radius of circle
How to calculae period in uniform circular motion
T = 2pi/w
How to calculate tangential (instantaneous) velocity in uniform circular motion
v = rw
How to calculate tangential acceleration in uniform circular motion
a = r alpha
angular motion kinematics equations
The same as linear just swap the variables
Centripetal acceleration
always points towards the center, a = v²/r
Centripetal force
Always points towards the center, maintains uniform circular motion, Fc = mv²/r
rotational kinetic energy
Krot = 1/2Iw^2²
torque
rotational force basically, t = rFsin(theta) or t = Ia
Simple harmonic motion position formula
x(t) = magnitude * cos( wt + shitf), period is T = 2pi/w
Spring period length
T = 2pisqrt(m/k)
Pendulum period length
T = 2pisqrt(l/g)
Universal Law of Gravitation
F = Gm1m2/r²
gravitational field strength/acceleration due to gravity
g = GM/r²
Gravitational Potential Energy
U = -GMm/r
Speed of orbiting Satellite
v² = gR²/r
Total Mechanical Energy in a system involving planets/sattelites
E = -GMm/2r
Escape Velocity
sqrt(2GM/r)
Kepler’s third law
R³/T² = a constant value