What is the relationship between escape velocity and gravitational forces?

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SUMMARY

The discussion clarifies the relationship between escape velocity and gravitational forces, emphasizing that escape velocity is defined as the speed at which the kinetic energy plus gravitational potential energy equals zero. The correct formula for escape velocity is V = √(2GM/r), which accounts for the balance between kinetic and potential energy. Participants highlighted the importance of understanding that an increase in velocity leads to elliptical orbits unless the velocity exceeds the escape threshold, allowing the object to overcome gravitational pull. The Virial Theorem was also referenced to explain the relationship between kinetic and potential energy in orbital mechanics.

PREREQUISITES
  • Understanding of gravitational forces and centripetal motion
  • Familiarity with kinetic and potential energy concepts
  • Knowledge of the Virial Theorem in physics
  • Basic algebra for manipulating equations
NEXT STEPS
  • Study the derivation of escape velocity using energy conservation principles
  • Explore the implications of the Virial Theorem in orbital mechanics
  • Learn about elliptical orbits and their characteristics in celestial mechanics
  • Investigate the effects of varying mass and distance on gravitational forces
USEFUL FOR

Students of physics, astrophysicists, and anyone interested in understanding orbital dynamics and the principles of escape velocity.

MRbrs
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Hi guys!

I want to ask something about escape velocity.

I know the definition of EV "escape velocity is the speed at which the kinetic energy plus the gravitational potential energy of an object is zero"(wikipedia).

Can we approach the problem by equalling the attractive force to the centrifugal force. I tried to find the the V in this way but I found the V \sqrt{2} times smaller. What is wrong with it?

mv^2/r = GmM/r^2

V=\sqrt{GM/r}

sorry about my poor English.
 
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When velocity is greater than the centripetal force, it just means that the path will not be circular, but it still can be an elliptical orbit. You need sufficient energy for the path to be a parabola or hyperbola.
 
I think when we increase the velocity of the object, centrifugal force becomes greater then attractive force so it escapes. However my equation is still false, why?
 
MRbrs said:
I think when we increase the velocity of the object, centrifugal force becomes greater then attractive force so it escapes. However my equation is still false, why?

The last post explained why. An increase in velocity will only increase in an elliptical orbit unless it is large enough.

Look at it this way: The object increases speed, so it begins to climb away. However, as it climbs it loses speed in exchange for gravitational potential. Eventually, it reaches a point where it loses enough speed that gravity starts to win the battle again and it begins to fall back. It gains speed at it falls, eventually returning to the point where it started and repeats the cycle again.

The only way that the object can completely escape is for the initial velocity increase to be large enough that the increase in altitude and corresponding decrease in gravity strength keeps ahead of the loss of velocity. This happens when:

V = \sqrt{\frac{2GM}{r}}
 
Thanks rcgldr and Janus for correcting me.

Velocity and force sometimes confuse me. I approached the concept of escape velocity as if the escape force. I guess the only way to determine the velocity is using the kinetic and the potential energies. So thanks again.
 
What you stumbled on with that radical-2 is Virial Theorem. It states that in any central potential for any closed orbit the average kinetic energy is minus a half of the average potential energy. In order for object to escape, kinetic energy must be equal to minus the potential energy.

In circular orbit, kinetic energy is always the same, so in order to double it, you must increase velocity by square root of 2. So that's exactly the factor by which escape velocity is different from velocity when centrifugal and gravitational forces are balanced.
 
k^2 said:
what you stumbled on with that radical-2 is virial theorem. It states that in any central potential for any closed orbit the average kinetic energy is minus a half of the average potential energy. In order for object to escape, kinetic energy must be equal to minus the potential energy.

In circular orbit, kinetic energy is always the same, so in order to double it, you must increase velocity by square root of 2. So that's exactly the factor by which escape velocity is different from velocity when centrifugal and gravitational forces are balanced.

Ok. I first write the equation of forces

mv^2/r = GmM/r^2

then multiplying both sides by r and dividing by 2

1/2 mv^2 = GmM/2r (The equation which you told)

V = \sqrt{GM/r}

this v is true when the objects are balanced. However to find the escape velocity I will have to balance the kinetic energy with potential energy. So I must multiply the velocity by sqrt of 2. Now, everything is clear. Thanks a lot to everyone.
 

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