Why do planets revolve in elliptical orbits?

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SUMMARY

Planets revolve in elliptical orbits due to Newton's law of gravitation, which states that the gravitational force is inversely proportional to the square of the distance (1/r²) between two objects. This mathematical framework predicts that objects under such gravitational influence will follow elliptical paths, with the larger mass located at one focus of the ellipse. While circular orbits occur under specific conditions of orbital speed, the predominant motion of planets around the sun is elliptical, influenced by the sun's mass and slight perturbations from other planets and relativistic effects.

PREREQUISITES
  • Newton's law of gravitation
  • Understanding of elliptical geometry
  • Basic principles of orbital mechanics
  • Familiarity with relativistic effects on gravity
NEXT STEPS
  • Study the mathematical derivation of elliptical orbits in classical mechanics
  • Explore the effects of gravitational perturbations in multi-body systems
  • Learn about the implications of general relativity on planetary motion
  • Investigate the conditions for circular orbits in celestial mechanics
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Astronomy students, physicists, and anyone interested in understanding the dynamics of planetary motion and gravitational interactions.

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we know that planets revolve in elliptical orbits but Why should planets revolve in elliptical orbits?
 
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spideyinspace said:
we know that planets revolve in elliptical orbits but Why should planets revolve in elliptical orbits?

It is a consequence of Newton's law of gravitation.
See e.g. here
 
spideyinspace said:
we know that planets revolve in elliptical orbits but Why should planets revolve in elliptical orbits?

In Newton's theory of gravity, the gravitational force on an object moving near a more massive object is proportional to 1/r^2 where r is the distance between the objects. When one works out mathematically the path for an object which is falling freely under the influence of such a force (but doesn't have enough energy to completely escape) the general answer is an ellipse where the large mass is at one focus.

There are of course some special cases; the obvious one is that if the orbital speed is just right for the distance, the path is a circle. Another is that if the falling mass is heading straight for the other mass, the path is a straight line downwards.

In the case of the planets, the sun is so much more massive than the planets that each planet basically moves in an ellipse around the sun, but the planets also have a very slight effect on the sun (especially Jupiter) and on each other, which distort the ellipses, and there are also other effects related to relativity which cause some further very slight distortions.
 

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