Derivation of Gravitational Potential

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Discussion Overview

The discussion revolves around the derivation of the gravitational potential formula, focusing on the mathematical steps involved in transitioning from the integral of gravitational force to the expression for gravitational potential energy. Participants explore the calculus required for this derivation and the conventions used in defining gravitational potential.

Discussion Character

  • Technical explanation
  • Mathematical reasoning
  • Conceptual clarification

Main Points Raised

  • One participant presents a derivation of gravitational potential energy, starting from the work-energy principle and integrating gravitational force.
  • Another participant questions how to proceed from the integral to the final expression, indicating a need for clarification on calculus techniques.
  • Several participants discuss the limits of integration, with one explaining that the potential is defined as the work done to bring an object from infinity to a distance R.
  • Another participant expresses uncertainty about pulling constants out of the integral and seeks confirmation on the reasoning behind the limit approaching zero as r approaches infinity.
  • A participant notes that the potential at infinity is conventionally defined as zero, emphasizing that this is a given rather than a derivable result.

Areas of Agreement / Disagreement

Participants generally agree on the mathematical steps involved in the derivation, but there is no consensus on the clarity of the calculus involved or the reasoning behind certain conventions. Some express uncertainty about specific aspects of the integration process.

Contextual Notes

Participants express varying levels of proficiency with calculus, which may affect their understanding of the integration steps. The discussion includes assumptions about the definition of gravitational potential and the limits of integration that are not universally accepted without further explanation.

Who May Find This Useful

This discussion may be useful for individuals studying gravitational physics, particularly those interested in the mathematical derivation of gravitational potential energy and the underlying calculus concepts.

AbsoluteZer0
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Hi,

The derivation of the Gravitational Potential formula, as I understand, is:

W = Fd (1)

W = G \frac{M_1m_2}{r^2}d (2) Substituting the Gravitational Force formula

W = - \int_R^∞G \frac{M_1m_2}{r^2} \, dr (3) Integrating within the boundaries of the initial distance (R) and Infinity

Which allows us to arrive at:

E_p = - \frac{GM_2m_1}{R} (4)

However, what I don't understand is how we are able to proceed from step 3 to step 4.
What method must be used in order to proceed as such?

My proficiency with Calculus is still in the works.

Thanks,
 
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Do you know how to do integrals like this one?

$$\int_a^b {x^n dx}$$

If so, here's a hint: ##\frac{1}{r^2} = r^{-2}##.

If no, then you'd best develop your calculus up to that point.
 
\lim_{t \to \infty} \int_{R}^{t} \frac{Gm_{1}m{2}}{r^{2}} dr

Do you know how to solve that?
 
Do you know how to do integrals like this one?

I can use integrals like these, to an extent.

Do you know how to solve that?

Unfortunately not.
 
\lim_{t \to \infty} -\int_{R}^{t} \frac{Gm_{1}m{2}}{r^{2}} dr
If you're taking an integral with respect to r and G, m1, and m2 are all constants, then what happens to the integral:
\lim_{t \to \infty} -Gm_{1}m_{2}\int_{R}^{t} \frac{1}{r^{2}}dr
Now take the fact that 1/r^2 = r^-2
So the integral is then solvable:
\lim_{t \to \infty} (-Gm_{1}m_{2} \frac{-1}{r})|_{t}^{R}
So then this becomes:
\lim_{t \to \infty} (\frac{-Gm_{1}m_{2}}{R}-\frac{-Gm_{1}m_{2}}{t})
Finally take the limit, anything over infinity tends to 0.
So you end up with:
\frac{-Gm_{1}m_{2}}{R}

Pretty sure the math is correct, someone might be able to fix any physics errors I have.
 
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Also, note that potential at infinity is conventionally defined to be 0. The convention, being what it is, isn't derivable mathematically, so you need to use it as a given in solving the problem when evaluating potential at infinity in your integral.

BiP
 
Quick question (for my knowledge), why are the limits of intergration from R to infinity?
 
iRaid said:
Quick question (for my knowledge), why are the limits of intergration from R to infinity?

The gravitationalpotential is defined as the work done by gravity to bring an object from infinity to a distance R from an object along a straight line, hence the limits of integration. A theorem from vector calculus shows that it does not matter what path the object travels, so the definition can be adjusted to an "arbitrary path from infinity to a distance R" from an object. But that is an offshoot of vector calculus.

BiP
 
I think I figured it out, please correct me if I'm wrong.

W = FdW = G\frac{M_1m_2}{r^2}dW =- \int_R^∞ G\frac{M_1m_2}{r^2}\,drW = - G M_1m_2 \int_R^∞ r^{-2}\,dr (Initially I was uncertain about pulling GM_1m_2 out)W = - G M_1m_2 [\frac{1}{r}]^R_∞
anything over infinity tends to 0.
Am I right in assuming that this is the reason why -G\frac{M_1m_2}{∞} produces zero? W = [-G \frac{M_1m_2}{r} - -G \frac{-GM_1m_2}{∞}]

Which leads to

E_p = -G\frac{M_1m_2}{r}

Thanks for the help
 
Last edited:

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