What is the kinetic energy when an object reaches escape velocity?

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SUMMARY

Escape velocity is the minimum speed required for an object to break free from the gravitational pull of a celestial body without any additional propulsion. It is defined mathematically by the equation \( v^2 = \frac{2GM}{r} \), where \( G \) is the gravitational constant, \( M \) is the mass of the celestial body, and \( r \) is the distance from the center of the body. As altitude increases, escape velocity decreases; for example, it is approximately halved at an altitude of 12,000 miles. The kinetic energy (KE) of an object at escape velocity is equal to the gravitational potential energy deficit, resulting in a net energy of zero when combined.

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  • Understanding of gravitational potential energy and kinetic energy concepts
  • Familiarity with the gravitational constant (G) and its significance
  • Basic knowledge of algebra and physics equations
  • Awareness of how altitude affects gravitational forces
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  • Study the derivation of escape velocity using gravitational potential energy equations
  • Explore the effects of air resistance on objects reaching escape velocity
  • Investigate how escape velocity varies for different celestial bodies
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Josielle Abdilla
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What is the kinetic energy equal to during the escape velocity? Henceforth, what is exactly happening at the escape velocity in terms of gravity?
 
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Josielle Abdilla said:
What is the kinetic energy equal to during the escape velocity? Henceforth, what is exactly happening at the escape velocity in terms of gravity?

Escape velocity is simply the velocity required for an object to escape the gravitational pull of a body, ignoring complications like air resistance and other gravitational-influencing bodies (Sun, Moon, other planets, etc). There is no 'during'. Escape velocity is not an event.

Nothing is happening to gravity in the context of escape velocity. The object is simply traveling so fast that the gravitational acceleration of the larger body cannot decelerate the object at a fast enough rate to ever pull the object back to the surface.
 
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Drakkith said:
Escape velocity is simply the velocity required for an object to escape the gravitational pull of a body, ignoring complications like air resistance and other gravitational-influencing bodies (Sun, Moon, other planets, etc). There is no 'during'. Escape velocity is not an event.

Nothing is happening to gravity in the context of escape velocity. The object is simply traveling so fast that the gravitational acceleration of the larger body cannot decelerate the object at a fast enough rate to ever pull the object back to the surface.
I would add that escape velocity decreases as altitude increases.

If you have an object exactly at escape velocity at the Earth's surface, it will still be exactly at "escape velocity" when it it 100 miles up. It will be going slower. Escape velocity 100 miles up is a bit slower than at the Earth's surface

If a quick calculation serves, escape velocity is cut approximately in half once an object is at 12,000 miles altitude (16,000 miles from the center of the Earth). Escape energy, aka potential energy deficit, scales inversely with distance from the center of the gravitating body. Quadruple the distance and you've cut energy by 1/4. So you've cut escape velocity by 1/2. The object will be moving half as fast as it was at the surface. And it will still be at escape velocity.

If it were to reach infinity without interference, an object that started at escape velocity at the Earth's surface would be at a dead stop. [Which is still equal to escape velocity because it would have already escaped]
 
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The KE of an mass at escape velocity is such that when its added to the gravitational potential energy of the mass, the result is zero.
In other words:
$$ \frac{mv^2}{2} - \frac{GMm}{r} = 0 $$

Thus:
$$ \frac{mv^2}{2} = \frac{GMm}{r} $$
$$ v^2 = \frac{2GM}{r} $$
 
Janus said:
The KE of an mass at escape velocity is such that when its added to the gravitational potential energy of the mass, the result is zero.
In other words:
$$ \frac{mv^2}{2} - \frac{GMm}{r} = 0 $$

Thus:
$$ \frac{mv^2}{2} = \frac{GMm}{r} $$
$$ v^2 = \frac{2GM}{r} $$
Note that this is using the definition of potential energy such that an object has zero potential at infinity, and increasingly negative potential as it approaches a massive object. This is a common definition, but certainly not the only definition, so you need to be a bit careful there.
 

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