Calculating Acceleration Due to Gravity in a Galaxy

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    Galaxy Gravity
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SUMMARY

The calculation of acceleration due to gravity within a galaxy differs significantly from the Earth-based formula GM/r². Instead, it involves the vector sum of gravitational forces from all mass distributions within the galaxy, where M represents the mass and r the distance to each mass. Astronomers utilize numerical simulations to estimate mass distribution, but these often fail to explain the observed acceleration of stars in the outer regions of galaxies. This discrepancy has led to theories such as dark matter and Modified Newtonian Dynamics (MOND) to explain the phenomenon.

PREREQUISITES
  • Understanding of gravitational force equations, specifically GM/r²
  • Familiarity with vector summation in physics
  • Basic knowledge of astronomical mass distribution
  • Awareness of dark matter and MOND theories
NEXT STEPS
  • Research numerical simulations for galaxy mass distribution estimation
  • Study the implications of dark matter on galaxy dynamics
  • Explore Modified Newtonian Dynamics (MOND) and its alternatives
  • Investigate General Relativity corrections in gravitational calculations
USEFUL FOR

Astronomers, astrophysicists, and students of physics interested in gravitational dynamics and the structure of galaxies will benefit from this discussion.

Bjarne
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Galaxy gravity ?

Which equation must be used to calculate Acceleration due to gravity inside a galaxy

I mean it is not the same as to calculate the acceleration towards the Earth GM/r2, - right ?
 
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Bjarne said:
Which equation must be used to calculate Acceleration due to gravity inside a galaxy

I mean it is not the same as to calculate the acceleration towards the Earth GM/r2, - right ?

Yes, apart from very small corrections for General Relativity, it's essentially the vector sum of that expression for each mass within the galaxy, where M is the mass and r is the distance to it, and the vector is in the direction of the mass.

That's obviously not very useful for practical purposes, so astronomers attempt to estimate the mass distribution at different positions within a galaxy and add up the effect, using numeric simulations if necessary.

When they do that, the result in most cases seems to be insufficient to account for the acceleration apparently being experienced by stars in the outer parts of galaxies. One theory to account for this discrepancy is the existence of "dark matter". Another class of theories (such as MOND) involves modifying gravity theory.
 

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