Calculate Real Freefall | GM/x^2 Integral

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SUMMARY

The discussion focuses on calculating real freefall using the variable acceleration formula GM/x² instead of the constant acceleration assumption. A participant outlines the integration process using Newton's second law, specifically applying radial components of force and velocity. The integration leads to the derivation of the kinetic energy formula (1/2 mv²) and gravitational potential energy from first principles, emphasizing the importance of understanding these concepts in the context of satellite orbits.

PREREQUISITES
  • Understanding of Newton's second law of motion
  • Familiarity with integral calculus
  • Knowledge of gravitational force equations
  • Basic principles of energy conservation in physics
NEXT STEPS
  • Study the derivation of gravitational potential energy for spherically symmetric bodies
  • Learn advanced integration techniques in calculus
  • Explore the dynamics of satellite motion and orbital mechanics
  • Investigate the implications of variable acceleration in physics problems
USEFUL FOR

Students in physics, particularly those studying mechanics and calculus, as well as educators looking to enhance their understanding of gravitational dynamics and energy conservation principles.

BoraDogan
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We always consider the accelaration as a constant thing, while calculating the freefall problems. What if we try to calculate the real. I mean taking the accelaration GM/x^2. I tried it but i could not handle that integral(Just graduated from high school). I would be happy if you reply.
Thank you
 
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BoraDogan said:
We always consider the accelaration as a constant thing, while calculating the freefall problems.
There are many problems that do not. We should have some older homework problems discussing this in our homework section.

Every satellite orbit is a related problem.
 
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There's a trick… Assuming no tangential component to the body's motion (as would be the case if it were released from rest) then, working with radial components of force and velocity, Newton's second law gives
[tex]\frac{GMm}{r^2}=-m\frac{dv}{dt}[/tex]
So[tex]\int{\frac{GMm}{r^2}}dr=-m\int{\frac{dv}{dt}dr}[/tex]
But [itex]\frac{dr}{dt}=v[/itex], so
[tex]\int{\frac{GMm}{r^2}}dr=-m\int{v\ dv}[/tex]

Both these integrations are easy. Either put limits in, or leave as indefinite integrals and find the value of the arbitrary constant afterwards.

You may well now realize that the result follows immediately from energy conservation. What I did above is to establish the [itex]\frac{1}{2}m\ v^2[/itex] kinetic energy formula (and that for gravitational PE due to a spherically symmetric body) from first principles, because doing this seemed more in the spirit of your question than simply quoting energy formulae.
 
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