Forest UCM Ch3 AngMom

Definition of Angular Momentum

The angular momentum of a single particle is defined as

[math]\vec \ell = \vec r \times \vec p[/math]

An coordinate must be defined in order to express the vectors for the particles position and momentum. The resulting angular momentum is defined with respect to the origin (rotation point) of the particle.

Torque

If I take the derivative of angular momentum with respect to time I get

[math]\vec{\dot \ell} = \frac{d}{dt} \left ( \vec r \times \vec p \right )[/math]

[math]= \left ( \vec \dot r \times \vec p \right ) + \left ( \vec r \times \vec \dot p \right )[/math]

[math] \left ( \vec \dot r \times \vec p \right )= \left ( \frac{1}{m} \vec p \times \vec p \right ) =0 [/math] cross product of parallel vectors

[math] \left ( \vec r \times \vec \dot p \right )=\left ( \vec r \times \vec F \right )= \vec \mathcal T[/math] Definition of Torque

[math]\vec \mathcal T =\vec{\dot \ell} [/math] Newton's second law for angular motion

Kepler's second Law

Kepler's second Law

A line segment joining a planet and the Sun sweeps out equal areas during equal intervals of time.

The above law is the result of the conservation of angular momentum when two bodies are attracted to eachother by a central force.

Consider a planet orbiting the Sun such that the sun if Fixed at the origin.

The line segment that joins the planet and the Sun is just the radius vector [math](\vec r )[/math] from the origin of a coordinate system where the sun is located to the position of the planet orbiting the sun.

The displacment vector for the planet is given as

[math]d \vec r = v dt[/math]

The differential area of the triangle representing a differential element of the orbital motion is given as

[math]dA = \frac{1}{2} \left | \vec r \times (\vec v dt ) \right | [/math]

Forest_UCM_MnAM#Angular_Momentum