Why Do Orbits Take an Elliptical Shape?

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SUMMARY

The orbits of celestial bodies are approximately elliptical due to the solutions of the Newtonian two-body problem, which yield conic sections. While the Sun's dominant mass influences the shape of these orbits, perturbations from other planets and the effects of general relativity cause minor deviations from perfect ellipses. Stable orbits are exclusively elliptical, as parabolic and hyperbolic orbits have been ejected from the solar system over time. Thus, the predominant orbital shape observed is elliptical.

PREREQUISITES
  • Newtonian mechanics
  • Conic sections in mathematics
  • General relativity basics
  • Two-body problem in physics
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  • Study the Newtonian two-body problem in detail
  • Explore the mathematical properties of conic sections
  • Investigate the effects of general relativity on planetary orbits
  • Research perturbation theory in celestial mechanics
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Astronomers, physicists, and students of celestial mechanics will benefit from this discussion, particularly those interested in the dynamics of planetary orbits and the underlying principles of gravitational interactions.

koolraj
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why are the orbits elliptical in shape?i know that force equations give differential equations whose solutions imply that the orbits elliptical in shape.but what is the particular physical reason behind it?
 
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You said it yourself: The solutions to the differential equations are ellipses. More precisely, the solutions to the Newtonian two-body problem are in the form of conic sections. Ellipses are one kind of conic section.

A better question: The solar system after all has more than two bodies in it, the whole solar system is orbiting the galaxy, and Newton's law of gravitation is only approximately correct. So why are orbits elliptical in shape?

The answer is that they aren't exactly elliptical in shape. They are instead approximately elliptical. The Sun is by far the dominant mass in the solar system. Planets perturb the orbits of each other from a purely elliptical shape. The primary effects are to slowly change the orientation and shape of the ellipse over time. General relativity similarly can be viewed, at least in our solar system, as a perturbative force. As far as the solar system orbiting the galaxy and the motion of the galaxy itself, those effects are so tiny as to be unmeasurable, at least as far as planetary orbits are concerned.
 
koolraj said:
why are the orbits elliptical in shape?i know that force equations give differential equations whose solutions imply that the orbits elliptical in shape.but what is the particular physical reason behind it?

I think it's worth nothing that the solution to the differential equations yields a conic section. The only stable orbits are ellipses, which is why all the planets approximately have this form. Everything that had a parabolic of hyperbolic orbit has long since been ejected from the solar system, leaving us to observe only ellipses.
 

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