B Celestial Mechanics: Eccentricity of Orbits

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    Eccentricity Orbits
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The discussion centers on whether an object in an eccentric orbit will become more circular over time, concluding that it will not, as eccentric orbits are stable solutions in celestial mechanics. The Earth's orbit does vary in eccentricity due to gravitational influences, particularly from non-spherical mass distributions. Tidal circularization can reduce eccentricity, especially in close satellite-primary systems, but this effect is contingent on the proximity and mass of the primary body. Gravitational interactions among moons can also prevent them from achieving circular orbits. Overall, while eccentricity can change due to specific factors, elliptical orbits remain stable and do not inherently decay towards circularity.
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a simple question about celestial mechanics...will the orbit of an object in an eccentric orbit become more circular over time, irrespective of impacts with other debris?
 
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No. An eccentric orbit is a stable solution to the equations of motion in a central force field.
 
@pixel - Consider:
The Earth's orbit varies over time in eccentricity from close to circular to mildly elliptic. Maybe that is what Madison Bond is referring to.
 
Hi madison:

What causes the eccentricity of an orbit (of a small mass object about a large mass object) to change is the lack of spherical symmetry in the larger mass object. The changes in the eccentricity of the moon's orbit is mostly due to the non-spherical symmetry of the Earth's gravitational field.

Regards,
Buzz
 
madison bond said:
a simple question about celestial mechanics...will the orbit of an object in an eccentric orbit become more circular over time, irrespective of impacts with other debris?
There is an effect called tidal circularization, in which tidal effects between the primary and the satellite work to reduce the eccentricity of the satellite. The strength of this depends on the proximity of the satellite and the mass of the primary. Jupiter has quite a strong effect on its inner satellites, and they have very small eccentricities. It is the gravitational interaction between the Moons themselves which prevent them from settling into circles.
 
jim mcnamara said:
@pixel - Consider:
The Earth's orbit varies over time in eccentricity from close to circular to mildly elliptic. Maybe that is what Madison Bond is referring to.

I was thinking of the ideal case of a particle in an inverse square force field.
 
I think @pixel answered the OP question correctly, as I get the impression that OP thinks that elliptical orbits are naturally decaying towards a circular one, whereas Kepler showed that they are stable.
 
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