Understanding Keplerian Orbits: Equations and Time Dependence

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SUMMARY

The discussion centers on the equations governing the displacement-time graph of Keplerian orbits. Participants confirm that the horizontal displacement is sinusoidal while the vertical displacement is cosinusoidal, or vice versa. The relationship between orbital angle and orbital radius is crucial for deriving the x/y components. However, the time dependence is implicit and requires complex differential equations for a complete understanding.

PREREQUISITES
  • Understanding of Kepler's laws of planetary motion
  • Familiarity with sinusoidal functions and their properties
  • Knowledge of differential equations
  • Basic concepts of orbital mechanics
NEXT STEPS
  • Study the derivation of Kepler's laws of planetary motion
  • Learn about the mathematical properties of sinusoidal and cosinusoidal functions
  • Explore advanced techniques in solving differential equations
  • Investigate the relationship between orbital angle and radius in detail
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Astronomy students, physicists, and mathematicians interested in orbital mechanics and the mathematical modeling of celestial bodies.

holtto
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Just curious, does anyone know what are the equations for the displacement-time graph of a Keplerian orbit?

The horizontal displacement-time graph should be somewhat sinusoidal, the vertical one cosinusoidal, or vice versa.
 
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There is a formula relating the orbital angle and the orbital radius, and so one can easily get the x/y components versus the angle. Dependence on time, however, is implicit.
 
voko said:
There is a formula relating the orbital angle and the orbital radius, and so one can easily get the x/y components versus the angle. Dependence on time, however, is implicit.

and it involves really complicated D.E.s
 

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