How is - (gravitational) potential energy and free fall compatible?

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Discussion Overview

The discussion revolves around the concept of negative gravitational potential energy and its compatibility with free fall. Participants explore the implications of gravitational potential energy in the context of motion towards a planetary body, examining reference points and the relationship between potential and kinetic energy.

Discussion Character

  • Exploratory
  • Technical explanation
  • Conceptual clarification
  • Debate/contested

Main Points Raised

  • One participant expresses confusion about negative gravitational potential energy and its relationship to acceleration towards a planetary body.
  • Another participant suggests that only the change in gravitational potential energy matters, noting that as one falls towards a planet, potential energy decreases while kinetic energy increases.
  • A participant questions whether gravitational potential energy is only zero at an infinite distance from a planetary body and discusses the implications of choosing different reference points for potential energy.
  • There is a mention of two reference points: one where potential energy approaches negative infinity as distance approaches zero, and another where potential energy is zero at infinity.
  • Another participant clarifies that choosing a reference point for potential energy is arbitrary and can be adjusted for convenience, such as setting potential energy to zero at the Earth's surface.

Areas of Agreement / Disagreement

Participants do not reach a consensus on the implications of negative gravitational potential energy or the best reference points for measuring it. Multiple competing views remain regarding the interpretation of potential energy in free fall.

Contextual Notes

Participants highlight the dependence on chosen reference points for gravitational potential energy and the potential confusion arising from different interpretations of these references. The discussion does not resolve the mathematical implications of these choices.

Who May Find This Useful

Readers interested in gravitational physics, potential and kinetic energy relationships, and the conceptual challenges of reference points in mechanics may find this discussion relevant.

FieldvForce
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I was having a few problems with Negative gravitational potential energy, I wasn't able to put my finger on why because it worked so well with everything else I had learned.

I tried to say it made sense because in space you don't free fall, but that's not actually true, though the gravitational energy is smaller you still accelerate (just very slightly) towards a planetary body.

If Ugrav is your store of potential KE, how can it be negative even in cases when you are accelerating towards a planetary body? This question has really slowed my studying down, help would be greatly appreciated.
 
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FieldvForce said:
If Ugrav is your store of potential KE, how can it be negative even in cases when you are accelerating towards a planetary body? This question has really slowed my studying down, help would be greatly appreciated.
All that matters is the change in gravitational PE. When you fall towards a planet,
you lose PE and gain KE. (The actual value of PE at any point is arbitrary and depends on what you chose as your reference point.)
 
Doc Al said:
All that matters is the change in gravitational PE. When you fall towards a planet,
you lose PE and gain KE. (The actual value of PE at any point is arbitrary and depends on what you chose as your reference point.)

I thought about this after I asked the question but I suspected that I had made another mistakeDo you mind confirming something for me.

The equation is derived (the way I learned it) by comparing the Ugrav of two positions and then making the second position (the final one) infinitely far from the center of the planetary object, does this mean that U is only 0 when r is infinity because there is no longer a difference between the Ugrav of the initial position and the final one?

And is U (as in Ui) always negative because the final position is made the reference position even though it's in the opposite direction of the centre if the planetary object.

It's cool that this equation has its reference point choosen as it forms, though this confused me as I thought the reference point was simply the centre of the Earth given the fact that the "work done" half of the equation was formulated using the centre as the ref.

Seems like there are two reference points one where U = minus infinity (r = 0) and U = 0 (r = infinity) however Ui being equal to minus infinity only means that it is inivity less than Uf right?

So for future reference the Ugrav of two or more objects are measured on a scale of 0 to infinity i.e relative to the position of the FINAL position from the deriving equation. God help me.

Also KE, when converted from U will move the object toward the Earth in the opposite direction of the reference point, thus it has potential to do negative work relative to the reference point.
 
Last edited:
You can choose any reference point and any finite value of U at that point. Choosing U = 0 when r = infinity is convenient for orbital mechanics, finding escape velocity, etc.

A reference point if "U = infinity when r = 0" doesn't really mean anything, because you can't do any sensible arithmetic with "infinity" (well, not without using some more devious math than you probably know about yet).

On the other hand, if you are dealing with motion close to the surface of the Earth and assuming gravitational acceleration is independent of altitude, it's simpler to take U = 0 at the surface of the Earth (or any other convenient altitude). That is where the formula "mgh" comes from, of course.
 
Thanks for all your help.
 

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