Modeling acceleration due to gravity for large bodies as a function of time

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SUMMARY

This discussion focuses on modeling the acceleration due to gravity for large bodies as a function of time, specifically using the equations GM/x²=A and Gm/x²=a. The conversation highlights the complexity of the problem, particularly when involving multiple bodies and vector quantities in three-dimensional space. A more accurate approach involves using integrated mass and density distributions rather than point mass. The differential form of Gauss' Law of Gravity, expressed as ∇·g = -4πGρ, is suggested as a foundational concept for deriving the gravitational vector field.

PREREQUISITES
  • Understanding of gravitational equations such as GM/x² and Gm/x²
  • Familiarity with vector calculus in three dimensions
  • Knowledge of Gauss' Law of Gravity and its differential form
  • Concept of mass density distributions in physics
NEXT STEPS
  • Study the application of Gauss' Law of Gravity in various contexts
  • Explore vector calculus techniques for modeling gravitational fields
  • Research integrated mass and density distribution methods in astrophysics
  • Learn about numerical methods for simulating multi-body gravitational interactions
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Physicists, astrophysicists, and students studying gravitational dynamics or anyone interested in advanced modeling of gravitational forces in multi-body systems.

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Given two bodies where GM/x^2=A and Gm/x^2=a, how might one model the acceleration of either bodies as a function of time?

A simpler version of the problem involves one of the masses being stationary (just for the sake of simplicity), so that GM/x^2=A and Gm/x^2=0.

A more complicated version would involve more than two bodies in multiple planes of space such that x1, x2, x3... etc. are vector quantities in 3 dimensions.

An even more complicated and accurate version would involve using integrated mass (taking into consideration the density distributions) instead of point mass.

I smell some serious calculus here but I can't wrap my head around how to do it. If anyone could explain how to do the simplest version or even what is involved that would be awesome. Also, any web resources on the kind of math involved or similar problems would be appreciated. Thanks!
 
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You could use the differential form of Gauss' Law of Gravity:

[tex]\nabla \cdot g = -4 \pi G \rho[/tex]

You would have to specify the mass density at each point on the masses, but then you can obtain the gravitational vector field for each mass. That might help you get started.
 

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