| Line 15: |
Line 15: |
| | An interesting case of a sideways force is a weight on the end of a string (like the Biblical slingshot used by [[David]] against [[Goliath]]). When you twirl the weight around above your head, the string is pulling the weight toward you - but it never gets any closer! This kind of force is called a [[centripetal force|centripetal]], or center seeking, force. | | An interesting case of a sideways force is a weight on the end of a string (like the Biblical slingshot used by [[David]] against [[Goliath]]). When you twirl the weight around above your head, the string is pulling the weight toward you - but it never gets any closer! This kind of force is called a [[centripetal force|centripetal]], or center seeking, force. |
| | | | |
| − | ==Angular momentum==
| + | SCIENCE IS USELESS! GOD>SCIENCE! |
| − | A rotating or orbiting body possesses angular momentum. Like linear momentum, angular momentum is a vector quantity and is conserved. An object's angular momentum changes only when a [[torque]] is applied to it.
| |
| | | | |
| − | The magnitude of the angular momentum of a particle orbiting some origin (such as the [[earth]] orbiting the [[sun]]) is given by
| |
| − |
| |
| − | :<math>L=mvr</math>
| |
| − |
| |
| − | where
| |
| − |
| |
| − | *'''L''' is angular momentum
| |
| − | *'''m''' is the mass of the particle
| |
| − | *'''v''' is the linear velocity of the particle
| |
| − | *'''r''' is the distance from the particle to the origin
| |
| − |
| |
| − | The direction of the angular momentum vector points perpendicularly to the plane formed by the object's orbit, in accordance with the [[right hand rule]].
| |
| − |
| |
| − | In addition to orbital angular momentum, the earth has rotational angular momentum due to its spin. The equations for calculating rotational angular momentum depend on the object's [[moment of inertia]], and therefore the shape and density of the object.
| |
| − |
| |
| − | === Generalized momentum ===
| |
| − | The definition of momentum can be generalized in [[Lagrangian Dynamics|Lagrangian]] and [[Hamiltonian Dynamics|Hamiltonian]] dynamics, to
| |
| − |
| |
| − | <math>
| |
| − | p=\frac{\partial L}{\partial \dot x}
| |
| − | </math>
| |
| − |
| |
| − | where L is the [[Lagrangian]] and <math>\dot x</math> is the velocity. In some cases the generalized momentum is the same as the momentum defined above. For example, for a free particle the Lagrangian equals the [[kinetic energy]] and so
| |
| − |
| |
| − | <math>
| |
| − | p=\frac{\partial (m\dot x^2/2)}{\partial \dot x}=m\dot x
| |
| − | </math>
| |
| − |
| |
| − | as above.
| |
| | ==External Links== | | ==External Links== |
| | *[http://id.mind.net/~zona/mstm/physics/mechanics/momentum/momentum.html Momemtum] | | *[http://id.mind.net/~zona/mstm/physics/mechanics/momentum/momentum.html Momemtum] |
| | | | |
| | [[Category:Physics]] | | [[Category:Physics]] |