Taylor series expansion for gravitational potential energy. GMm/r=mgh near the earth

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Discussion Overview

The discussion centers on the Taylor series expansion of the gravitational potential energy equation, specifically the relationship GMm/r = mgh for distances close to the Earth. Participants explore the implications of using a first-order Taylor expansion and the significance of higher-order terms in this context.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested

Main Points Raised

  • Some participants question the validity of using only the first-order Taylor expansion, suggesting that it may not capture the complete function and that the error of the polynomial has not been bounded.
  • Others argue that higher-order terms become insignificant when h/R is much less than 1, implying that they can be safely ignored in practical applications.
  • There is a suggestion that the second-order term could be considered to assess its impact relative to the first-order term, particularly in terms of error margins.
  • One participant notes that if h/R is very small, the succeeding terms in the expansion decrease rapidly, making them negligible.
  • Another participant acknowledges that U = mgh is a good approximation for gravitational potential energy when h is small compared to R, but not an exact representation.

Areas of Agreement / Disagreement

Participants express uncertainty regarding the sufficiency of the first-order Taylor expansion, with some advocating for its use while others emphasize the importance of considering higher-order terms. The discussion remains unresolved regarding the completeness of the approximation.

Contextual Notes

Limitations include the dependence on the assumption that h is much smaller than R, and the lack of a formal error analysis for the polynomial approximation.

CrazyNeutrino
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Using taylor series expansion to prove gravitational potential energy equation, GMm/r=mgh at distances close to the earth.
R= radius of the Earth h= height above surface of the Earth m= mass of object M= Mass of the earth

U = - GmM/(R + h)

= - GmM/R(1+ h/R)

= - (GmM/R)(1+ h/R)^-1

do a binomial expansion or Taylor's series with (h/R) as the small variable;

= -(GmM/R)[1 - (h/R) + ...].

DOUBT: In this step why do we only use the FIRST order taylor expansion and no more?
The function would not be complete would it?and nothing has been done to bound the error of the polynomial. Why would taking the first non-trivial term (first order term) of the expansion of 1+x (that is 1-x) account for the entire function 1+x or in this case 1+h/r.

PLEASE REPLY ...

Proof (continued): -(GMm/R)(1-(h/R)= -(GmM/R) + GmMh/R^2

In the second term note that GM/R^2 =g

= - (GmM/R) + mgh

So the potential energy at "r" can be written as PE at "R" plus PE at "h"

Now in planetary problems, where the distance h is not small and you use the general formula - GmM/r it is convienient to choose U = 0 at r = infinity
However near the Earth we can arbitrarily chose U=0 at U = - (Gmm/r)

Therefore: U = mgh when h<<<R
 
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CrazyNeutrino said:
DOUBT: In this step why do we only use the FIRST order taylor expansion and no more?
The function would not be complete would it?and nothing has been done to bound the error of the polynomial. Why would taking the first non-trivial term (first order term) of the expansion of 1+x (that is 1-x) account for the entire function 1+x or in this case 1+h/r.
Succeeding terms would be higher order powers of h/R and thus increasing insignificant when h/R << 1.
 


Wouldn't that mean that h/r would be off by all the succeeding terms all the way to infinity?
 


CrazyNeutrino said:
DOUBT: In this step why do we only use the FIRST order taylor expansion and no more?
The function would not be complete would it?and nothing has been done to bound the error of the polynomial. Why would taking the first non-trivial term (first order term) of the expansion of 1+x (that is 1-x) account for the entire function 1+x or in this case 1+h/r.

If you're worried, you can write down the second order term, and then figure out what condition needs to hold in order for the second order term to be at most, say, 1% of the first order term.
 


Okay... So your trying to imply that when h/r is way less than 1, higher order powers of h/r increase it insignificantly?
 


CrazyNeutrino said:
Wouldn't that mean that h/r would be off by all the succeeding terms all the way to infinity?
The terms get smaller and smaller, so they can be safely ignored.

Imagine if h/R = 1/1000

Then (h/R)2 = 10-6, (h/R)3 = 10-9, and so on.

Write out the next few terms of the expansion and see how small they are compared to the first.
 


Thanks a lot! That explains it.
 


Also that implies that U = mgh is just an incredibly good approximation right? Not exactly the potential energy.
 


CrazyNeutrino said:
Also that implies that U = mgh is just an incredibly good approximation right? Not exactly the potential energy.

Yes. It's a good approximation anytime that h (which is really the difference between two values of the distance from the center) is small compared with the distance from the center. This will be the case for most reasonable heights from the surface of the earth.
 

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