Non-equal Gravitational Potential and Kinetic Energy in a closed system

Click For Summary

Discussion Overview

The discussion revolves around the concepts of gravitational potential energy and kinetic energy in a closed system involving two point masses. Participants explore the calculations of gravitational forces, potential energy, and kinetic energy as the masses move towards each other over time. The scope includes theoretical reasoning and mathematical calculations related to gravitational interactions.

Discussion Character

  • Exploratory
  • Technical explanation
  • Mathematical reasoning
  • Debate/contested

Main Points Raised

  • One participant describes a system with two point masses and calculates the gravitational forces and potential energy, noting a discrepancy in energy conservation.
  • Another participant challenges the initial force calculations, asserting that the forces must be equal due to Newton's third law.
  • There is a discussion about the correct way to calculate gravitational potential energy, with a later reply providing the formula U = -Gm1m2/r.
  • Participants express concerns about discrepancies in kinetic energy calculations compared to potential energy changes, questioning the significance of the resulting energy difference.
  • One participant suggests that the observed discrepancies might be due to rounding errors in calculations.

Areas of Agreement / Disagreement

Participants generally disagree on the calculations of forces and potential energy, with multiple competing views on how to approach the problem. The discussion remains unresolved regarding the discrepancies in energy calculations.

Contextual Notes

Limitations include potential rounding errors in calculations and the need for clarity on the definitions and assumptions used in the energy calculations. The discussion highlights the complexity of gravitational interactions and energy conservation in a closed system.

FlipC
Messages
4
Reaction score
0
While trying to get my head around Gravitational Potential Energy I devised the following simple system:

Point Mass A of 1kg is 1000m away from Point Mass B of 100kg within an empty universe.

The gravitational force exerted by A on B is G*10^-16; by B on A is G*10^-4. At time=0 these two unmoving bodies possesses no kinetic energy. Both posses the same amount of gravitational potential energy (mgh) with respect to each other of G*10^-1.

At t=1 second they've attracted each other and moved closer. Body A at a speed of G*10^-4 and B at a speed of G*10^-8. They therefore posses kinetic energy equal to .5mv^2. Their potential energy has also changed due to both the reduced distance and the increase in relative gravities.

However when I run the figures I end up with ~2.2*10^-29 Joules over.

Given the tiny value it may be rounding errors in my calculation programme or a flaw in my basic assumptions, but if not where has this energy come from?
 
Last edited:
Physics news on Phys.org
FlipC said:
The gravitational force exerted by A on B is G*10^-16; by B on A is G*10^-4.
How did you calculate this? They must exert the same force on each other. (Newton's 3rd law.)

At time=0 these two unmoving bodies possesses no kinetic energy. Both posses the same amount of gravitational potential energy (mgh) with respect to each other of G*10^-1.
The gravitational PE belongs to the system of both bodies, not to each individually. (And you cannot use 'mgh' to calculate it, of course.)

At t=1 second they've attracted each other and moved closer. Body A at a speed of G*10^-4 and B at a speed of G*10^-8.
Since momentum is conserved, their speeds will always be such to give zero total momentum.
 
Doc Al said:
How did you calculate this? They must exert the same force on each other. (Newton's 3rd law.)

Tcch yeah just realized that, force = G*10^-4 with speeds of G*10^-4 and G*10^-6 respectively.

The gravitational PE belongs to the system of both bodies, not to each individually. (And you cannot use 'mgh' to calculate it, of course.)

PE with relation to what and how is it then calculated?
 
FlipC said:
PE with relation to what and how is it then calculated?
The gravitational PE of the system is given by:
U = - \frac{Gm_1m_2}{r}
 
Okay having calculated that at t=0 and t=1 determine KE at both times as well. I still get a discrepancy. There's more KE than be accounted for by the change in PE by 2.2*10^-29J
 
FlipC said:
Okay having calculated that at t=0 and t=1 determine KE at both times as well. I still get a discrepancy. There's more KE than be accounted for by the change in PE by 2.2*10^-29J
How are you doing your calculation? How far have the bodies moved? What's the change in PE? (Is 2.2*10^-29J significant or just a trivial difference due to round off?)
 
After 1 second Body A will be traveling at G*10^-4 m/s and Body B at G*10^-6 m/s. Assuming linear acceleration the distance between them will have reduced by (G*10^-4+G*10^-6)/2 m.

Calculate PE and KE at t=0 and t=1. Given a closed system the difference in sum of energies at each point should be zero; except I keep getting that difference in total KE being higher than total PE.

Hmm okay writing that out again. Gravity changes with distance therefore the acceleration changes such that the bodies move faster and the distance increases more. However it still seems that the ratios between them produce a higher KE than allowed for by the change in PE.

As I said it may well be a rounding error.
 

Similar threads

  • · Replies 9 ·
Replies
9
Views
2K
  • · Replies 2 ·
Replies
2
Views
2K
  • · Replies 54 ·
2
Replies
54
Views
7K
  • · Replies 46 ·
2
Replies
46
Views
5K
  • · Replies 29 ·
Replies
29
Views
4K
  • · Replies 6 ·
Replies
6
Views
2K
  • · Replies 3 ·
Replies
3
Views
2K
  • · Replies 10 ·
Replies
10
Views
2K
  • · Replies 3 ·
Replies
3
Views
2K
  • · Replies 16 ·
Replies
16
Views
3K