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List Of Equations In Classical MechanicsThis page gives a summary of important equations in classical mechanics. Nomenclature - a = acceleration (m/s²)
- F = force (N = kg m/s²)
- KE = kinetic energy (J = kg m²/s²)
- m = mass (kg)
- p = momentum (kg m/s)
- s = position (m)
- t = time (s)
- v = velocity (m/s)
- v0 = velocity at time t=0
- W = work (J = kg m²/s²)
- s(t) = position at time t
- s0 = position at time t=0
- runit = unit vector pointing from the origin in polar coordinates
- θunit = unit vector pointing in the direction of increasing values of theta in polor coordinates
Note: All quantities in bold represent vectors. Defining Equations Center of Mass In the discrete case: -
where is the number of mass particles. Or in the continuous case: -
where ρ(s) is the scalar mass density as a function of the position vector. Velocity -
-
Acceleration -
-
-
(R = radius of the circle, ω = v/R angular velocity) Momentum -
Force -
- (Constant Mass)
Impulse -
- if F is constant
Moment of Intertia For a single axis of rotation: Angular Momentum - if v is perpendicular to r
Vector form: -
(Note: I can be treated like a vector if it is diagonalized first, but it is actually a 3×3 matrix) r is the radius vector Torque -
-
if |r| and the sine of the angle between r and p remains constant. -
This one is very limited, more added later. α = dω/dt Precession Energy -
- if m is constant
- (near the earth's surface)
g is the acceleration due to gravity, one of the physical constants at or near the earth's surface. Central Force Motion -
Gravitational Force -
- G is the gravitational constant, one of the physical constants
Useful derived equations Position of an accelerating body - if a is constant.
Equation for velocity -
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