Escape velocity and kinetic energy of the Earth

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Discussion Overview

The discussion revolves around the concept of escape velocity and the kinetic energy associated with two masses in a gravitational interaction, particularly focusing on the case of an object escaping Earth's gravitational pull. Participants explore the implications of mass interactions, gravitational potential, and the role of kinetic energy in these scenarios.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested
  • Mathematical reasoning

Main Points Raised

  • One participant questions why the escape velocity formula for an object on Earth only considers the object's kinetic energy and not that of the Earth, suggesting that the Earth's kinetic energy might be negligible due to conservation of momentum.
  • Another participant notes that the gravitational potential equation typically assumes a small mass and a large mass, with the large mass not moving, and suggests that different equations apply when both masses are of similar size.
  • A participant emphasizes that kinetic energy is proportional to the square of velocity, indicating that the distribution of energy between two masses depends on their mass ratio and velocities.
  • There is a request for clarification on deriving the gravitational potential when both objects move different distances, highlighting the complexity of calculating work done on them.
  • One participant expresses confusion about their approach, stating that they consistently find the kinetic energy of one mass equaling the potential energy of the system, which they believe cannot be correct.
  • Another participant suggests looking into the concept of "reduced mass" as a potential avenue for resolving the confusion regarding energy calculations.

Areas of Agreement / Disagreement

Participants express differing views on the treatment of kinetic energy in gravitational interactions, particularly regarding the assumptions made about mass sizes and movement. The discussion remains unresolved, with multiple competing perspectives on how to approach the calculations and concepts involved.

Contextual Notes

Participants highlight limitations in their understanding of the derivation of gravitational potential when both masses are significant, as well as the implications of conservation of momentum in energy distribution. There are unresolved mathematical steps and assumptions that affect the clarity of the discussion.

Alexander350
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If you had two masses, m_{1} and m_{2}, and you released them in space infinitely far apart, their kinetic energies would satisfy \frac{1}{2}m_{1}v_{1}^2+\frac{1}{2}m_{2}v_{2}^2=\frac{Gm_{1}m_{2}}{r} if they met with a distance r between their centres of mass. This equation therefore tells you the velocities needed for the two bodies to escape the gravitational pull of each other, i.e. the escape velocities. So, why does the formula for the escape velocity of an object on Earth only include the kinetic energy of the object, and not the Earth itself? Is the kinetic energy of the Earth just negligibly small (because the conservation of momentum means its velocity is pretty much zero) and can therefore be ignored? Would it only be necessary if the two objects had similar mass?
 
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The equation you are used to for the gravitational potential assumes a small mass and a large mass, where the large mass is assumed not to move. If you have two masses of a similar relative size, then you have a different equation for the gravitational potential of the system. You might like to derive it as a useful exercise.
 
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Alexander350 said:
Is the kinetic energy of the Earth just negligibly small (because the conservation of momentum means its velocity is pretty much zero) and can therefore be ignored?
The momentum is proportional to the velocity but the KE is proportional to the velocity squared. So the sharing of the available energy into the KE of each object is proportional to the square of the ratio of the velocities and inversely with the ratio of the masses. Velocity wins.
 
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PeroK said:
The equation you are used to for the gravitational potential assumes a small mass and a large mass, where the large mass is assumed not to move. If you have two masses of a similar relative size, then you have a different equation for the gravitational potential of the system. You might like to derive it as a useful exercise.
I have been thinking about this for a while and am still not sure how to derive it. The problem is that both the objects move different distances, so how can you calculate the work done on them?
 
Alexander350 said:
I have been thinking about this for a while and am still not sure how to derive it. The problem is that both the objects move different distances, so how can you calculate the work done on them?

Look at how the force acts over a small distance. Don't forget conservation of momentum, which relates the velocities of the two masses.
 
PeroK said:
Look at how the force acts over a small distance. Don't forget conservation of momentum, which relates the velocities of the two masses.
Even trying to use conservation of momentum, I always end up with the kinetic energy of one of the masses equalling the potential energy of the system. This cannot be right as then there would be twice as much energy as there actually is. How do I set up the equations as I am obviously approaching it wrong.
 
Alexander350 said:
Even trying to use conservation of momentum, I always end up with the kinetic energy of one of the masses equalling the potential energy of the system. This cannot be right as then there would be twice as much energy as there actually is. How do I set up the equations as I am obviously approaching it wrong.

If you want to work this out yourself you should post it as homework and show your working.

Otherwise you could look up "reduced mass".
 
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