The spherical symmetry of massive bodies

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SUMMARY

The discussion focuses on the gravitational interaction between two bodies with non-spherical symmetry, specifically addressing the Earth and the Moon. It establishes that if one mass is spherical, its gravitational field can be calculated easily, while a non-spherical mass requires numerical integration to determine the net force acting on it. This method, described as "brute force," effectively calculates gravitational interactions without approximations. The conversation highlights the limitations of approximating small bodies in a parallel force field, emphasizing the need for precise calculations in astronomical contexts.

PREREQUISITES
  • Understanding of gravitational forces and fields
  • Familiarity with numerical integration techniques
  • Knowledge of spherical and non-spherical mass distributions
  • Basic principles of celestial mechanics
NEXT STEPS
  • Research numerical integration methods for gravitational fields
  • Study the effects of non-spherical mass distributions in celestial mechanics
  • Explore computational tools for simulating gravitational interactions
  • Learn about the gravitational field of irregularly shaped bodies
USEFUL FOR

Astronomers, physicists, and students studying gravitational interactions and celestial mechanics will benefit from this discussion, particularly those interested in the complexities of non-spherical mass distributions.

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Homework Statement



Consider the study of the motion of a two bodies system interacting with only gravitational forces.
If the two bodies (or even one of them) has not spherical symmetry, how will you proceed? Indeed the Earth and the moon does not have spherical symmetry mass distributions but normally we consider them as..
thank you



Homework Equations





The Attempt at a Solution



 
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If one of the masses is spherical, you can easily find its gravitational field. Then you place the non-spherical mass in that field and do a numerical integration to find the net force on it. If the first mass is not spherical, then you first need to do a numerical integration to find its gravitational field.

This "brute force" method will work with any mass and requires no approximations or assumptions. It basically calculates the net force between the two masses by adding over all possible pairs dm1 and dm2.
 
Thank you, I've understand.
It is true that if the body is small enough it can be considered set in a field of parallel forces (with obvious and simple results) but this is an approximation that works fine, i think, for artificial satellites and for the bodies on a 'human scale'.
In astronomical calculations on the motions of planets and satellites, however, I wonder how it is take in account the 'non-symmetry' of bodies.
Do you know any reference?
 

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