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About EP 222: Classical Mechanics Tutorial Sheet 3
1) The radial position of a satellite perturbed from a circular orbit will execute simple harmonic motion with an angular frequency equal to the square root of the planet's gravitational parameter divided by the cube of the initial orbital radius. 2) For a particle under an inverse cube central force, it will move in a circular orbit when its angular momentum is equal to the mass of the particle times the force constant. 3) Integrating the differential equation relating the radial and angular coordinates directly yields the same orbital equation as solving the differential equation for the reciprocal of the radial coordinate.
Detailed Information
| Author: | ['haroldo'] |
|---|---|
| Publication Year: | 2020 |
| Pages: | 12 |
| Language: | English |
| Format: | |
| Price: | FREE |
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