| Laplace-runge-lenz Vector |
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Information AboutLaplace-runge-lenz Vector |
| CATEGORIES ABOUT LAPLACE-RUNGE-LENZ VECTOR | |
| classical mechanics | |
| celestial mechanics | |
| rotational symmetry | |
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: where:
The Laplace-Runge-Lenz vector is constant for the motion of a particle acted on by a Central Force that varies as an inverse square (e.g., Gravity and Electrostatics ), i.e., for Potential s that vary as . PROPERTIES By its definition, is perpendicular to (i.e., ). (Recall that , because ). The Laplace-Runge-Lenz vector can be used to derive the elliptical orbits of the Kepler problem : where is the angle between the position and Laplace-Runge-Lenz vectors. Permuting the Triple Dot Product and rearranging yields the formula for an Ellipse : The vector points toward the Pericenter , from the geometric center of the orbit to the attracting, central body. The magnitude for a Periodic Orbit with Eccentricity is given by: |
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