What is the time taken to reach a given height with escape velocity?

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SUMMARY

The time taken to reach a given height when launched at escape velocity from Earth's surface involves complex gravitational dynamics. The acceleration is determined by the formula F = -GMm/r², where G is the universal gravitational constant, m is the object's mass, M is Earth's mass, and r is the distance from Earth's center. The integration of velocity and distance leads to an elliptic integral, which is not solvable using elementary functions but is well-documented in mathematical tables. Starting at escape velocity simplifies the integral, allowing for easier calculations.

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If an object is launched at escape velocity from the surface of the Earth, how long will it take to reach a given height h? Ignoring air resistance and other gravity, etc.
 
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That sounds like a pretty basic problem but it isn't, quite. For motion near the surface of the earth, we could take the acceleration due to gravity to be constant, -g. But if you are talking about "escape velocity" you must be considering the object moving to great distance compared to the radius of the earth. Then F= -GmM/r^2 where G is the "universal gravitational constant", m is the mass of the object, M is the mass of the earth, and r is the distance from the center of the earth, so that the acceleration is -GM/r^2.

That gives a= dv/dt= -GM/r^2. Since the variables on the left are "v" and "t" while we have "r" on the right (and v= dr/dt), we can use a technique called "quadrature". Since a= dv/dt= (dv/dr)(dr/dt) (by the "chain rule") a= (dv/dr)(dr/dt)= (dv/dr)v= -GM/r^2. We can write that as v dv= (-GM/r^2)dr.


Integrating (1/2)v^2= GM/r+ C (That, by the way, is "conservation of energy"- the left is kinetic energy, the right is the negative of the potential energy, and there difference is constant). Then we have v^2= 2GM/r+ C so that v= dr/dt= \sqrt{2GM/r+ C}.

Now, we need to integrate \frac{dr}{\sqrt{2GM/r+ C}}= dt.

The left side is an "elliptic integral" (from the fact that it is related to calculating the orbits of planets and satellites which are ellipses), well known NOT to be integrable in terms of elementary functions but well tabulated.
 
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If you start at scape velocity, than the constant C vanishes (Which is just the total mechanical energy) vanishes and the integral can be easily performed.
 

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