Escape velocity and kinetic energy of the Earth

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SUMMARY

The discussion centers on the derivation of escape velocity and kinetic energy in a two-body system, specifically addressing the gravitational interaction between two masses, m1 and m2. The key equation presented is \(\frac{1}{2}m_{1}v_{1}^2+\frac{1}{2}m_{2}v_{2}^2=\frac{Gm_{1}m_{2}}{r}\), which illustrates the velocities required for escape. Participants question why the kinetic energy of the Earth is often neglected in calculations, attributing this to its relatively small velocity due to conservation of momentum. The discussion also highlights the importance of understanding gravitational potential in systems with similar mass sizes.

PREREQUISITES
  • Understanding of Newton's laws of motion
  • Familiarity with gravitational potential energy concepts
  • Knowledge of kinetic energy equations
  • Basic grasp of conservation of momentum principles
NEXT STEPS
  • Research "reduced mass" and its application in two-body problems
  • Learn about gravitational potential energy in systems with equal masses
  • Explore the derivation of escape velocity for two-body systems
  • Study the implications of conservation of momentum in gravitational interactions
USEFUL FOR

Students of physics, astrophysicists, and anyone interested in understanding gravitational interactions and escape velocity calculations in two-body systems.

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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