Ridiculously difficult Newtonian physics problem

Join the discussion
Ask a follow-up here, or get your own question answered by working scientists, mathematicians and engineers — people, not an autocomplete.
Real named experts · corrections over time · the nuance an AI answer skips
12 replies · 3K views
Mason Pulinthanathu
Messages
5
Reaction score
0
Homework Statement
Derive n expression for the time for an object to move in space from point a to b as a result of the gravitational force of another object
Relevant Equations
MmG/r^2=F | -MmG/r=PE| PE1+KE1=PE2+KE2
physics.PNG
I have been trying out with this one for a long time with no luck getting the exact expression. I am pretty sure this is somehow related to Kepler's third law but unable to establish the connection and the integrals I get from energy conservation yield different results. Any ideas?
 
Physics news on Phys.org
geekmohmmad said:
Homework Statement:: Derive n expression for the time for an object to move in space from point a to b as a result of the gravitational force of another object
Relevant Equations:: MmG/r^2=F | -MmG/r=PE| PE1+KE1=PE2+KE2

View attachment 257518I have been trying out with this one for a long time with no luck getting the exact expression. I am pretty sure this is somehow related to Kepler's third law but unable to establish the connection and the integrals I get from energy conservation yield different results. Any ideas?
This is quite a well known problem. What do you know about differential equations?

Conservation of energy should give you a differential equation to get you started.
 
  • Love
Likes   Reactions: Mason Pulinthanathu
You're right, this is a ridiculously difficult problem.
It's a non-linear ODE whether you approach it from force, or from energy as post 2 suggests.
Wolfram Alpha gives you an answer for the force way. Ugly!
Then you have r(t) but you want t(r).
That's the best I can think of.
My sympathies!
 
  • Love
Likes   Reactions: Mason Pulinthanathu
Since you are given the solution and are only asked to show it is correct, "all" you need to do is to demonstrate that it satisfies the differential equation and boundary conditions.
 
  • Love
  • Informative
Likes   Reactions: Neeleshatom and Mason Pulinthanathu
87296234_486183958955103_6013091949706215424_n.jpg

Thanks all for the responses. I think this the right path to derive it, but I am unable to solve this integral.
 
PeroK said:
This is quite a well known problem. What do you know about differential equations?

Conservation of energy should give you a differential equation to get you started.
Thank you for the response. I have a solid understanding of Calc 1 and can solve basic differential equations. Can you help me please with this integral?
87296234_486183958955103_6013091949706215424_n.jpg
 
rude man said:
You're right, this is a ridiculously difficult problem.
It's a non-linear ODE whether you approach it from force, or from energy as post 2 suggests.
Wolfram Alpha gives you an answer for the force way. Ugly!
Then you have r(t) but you want t(r).
That's the best I can think of.
My sympathies!
I would be really thankful if you could send me the Wolfram Alpha solution. Thanks in advance.
 
geekmohmmad said:
I would be really thankful if you could send me the Wolfram Alpha solution. Thanks in advance.
You 'loved' my post #4 but did not act on it.
There's a fairly obvious trig substitution that makes the RHS of the expression for t much simpler. Differentiating that leads in a few lines to the energy equation. You can then reverse the process to see how the ODE can be solved.
 
  • Like
Likes   Reactions: Mason Pulinthanathu, Vanadium 50 and etotheipi
geekmohmmad said:
Thank you for the response. I have a solid understanding of Calc 1 and can solve basic differential equations. Can you help me please with this integral? View attachment 257578

You have:
$$\frac{dr}{dt} = -\sqrt{2GM(\frac 1 r - \frac 1 {r_1}) }= -\sqrt{2GM(\frac{r_1 - r}{rr_1})}$$
$$-\int_{r_1}^{r_2} \sqrt{\frac{rr_1}{r_1 - r}} dr =\int_0^{t_2}\sqrt{2GM}dt = t_2\sqrt{2GM}$$
Note that I've used ##r_2## as the final radius to avoid confusion with the variable ##r##.

The key to such integrals is to look for a suitable trig substitution. You might look first at ##r = r_1\cos \theta##, which works for an inverse cube law problem. That doesn't quite work here. Any inspiration?
 
Last edited:
  • Like
Likes   Reactions: Mason Pulinthanathu and etotheipi
PeroK said:
You have:
$$\frac{dr}{dt} = \sqrt{2GM(\frac 1 r - \frac 1 {r_1}) }= \sqrt{2GM(\frac{r_1 - r}{rr_1})}$$
Shouldn't there be a negative sign in front of the radical? The radial distance ##r## is positive and ##\dfrac{dr}{dt}## must be negative since ##r## decreases with time. This means choosing the negative sign when taking the square root.
 
  • Like
Likes   Reactions: Mason Pulinthanathu and PeroK
kuruman said:
Shouldn't there be a negative sign in front of the radical? The radial distance ##r## is positive and ##\dfrac{dr}{dt}## must be negative since ##r## decreases with time. This means choosing the negative sign when taking the square root.
Very true. I was trying to adjust my solution to the OP's notation and forgot about that.
 
  • Like
Likes   Reactions: Mason Pulinthanathu
PeroK said:
Very true. I was trying to adjust my solution to the OP's notation and forgot about that.
Thanks for the reply. Here what I've done. (Have no clue how to un-substitute or what to do after this!)
integration.PNG
 
That doesn't look quite right. For example, ##1 - \frac{r_1}{r}## is negative, but you have it in a square root.

You are making things much more difficult than they need be.

I showed you how to simplify that expression with the square roots on the denominator. Also, you have used:
$$\frac 1 r = \frac 1 {r_1} \sec^2 \phi$$
Which is more simply written as:
$$r = r_1 \cos^2 \phi$$

I would start with the simplified expression in the integral I gave you:

PeroK said:
$$-\int_{r_1}^{r_2} \sqrt{\frac{rr_1}{r_1 - r}} dr =\int_0^{t_2}\sqrt{2GM}dt = t_2\sqrt{2GM}$$

And try the substitution ##r = r_1 \cos^2 \theta##. Or use ##\phi## is you prefer.