Online Encyclopedia
List of equations in classical mechanics
This page gives a summary of important equations in classical mechanics.
Contents |
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 n 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
- Centripetal 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
- iff 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 the physical constants.
Central Force Motion
Useful derived equations
Position of an accelerating body
- if a is constant.
Equation for velocity
Last updated: 01-22-2005 01:27:38