Minimum velocity to throw a object to another planet

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Homework Help Overview

The discussion revolves around determining the minimum velocity required to throw an object from one planet to another, considering gravitational interactions. The problem involves concepts from gravitational physics, work-energy principles, and potential energy calculations.

Discussion Character

  • Exploratory, Conceptual clarification, Mathematical reasoning, Assumption checking

Approaches and Questions Raised

  • Participants explore integrating work done by gravitational forces and potential energy changes. Questions arise about the relevance of certain integrals and the symmetry of the gravitational influences from both planets.

Discussion Status

There is an ongoing exploration of various mathematical approaches, with some participants suggesting that potential energy should be considered instead of work. Multiple interpretations of the problem setup are being discussed, particularly regarding the distances involved and the nature of the trajectory.

Contextual Notes

Participants express uncertainty about the distances between the planets and the implications of those distances on the problem. There are also mentions of potential divergences in integrals and the need for clarity on the physics involved in projectile motion between two planets.

  • #31
PeroK said:
Nevertheless the answer you are aiming for is wrong.

If D is small, then as mentioned above you have a very different problem.

I'm not sure what else to suggest.
I'll try what jbriggs444 suggested about adding energies
 
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  • #32
Highway_Dylan said:
The answer I got is:

## v_0^2=2GM\frac{(D+R)^2}{R(D+2R)(D+3R)}##.

Liable to my own algebraic error of course. I hope that posting this is allowed, since OP showed that he has the intended final answer available.
Yes, that's the answer I get also, assuming that D is the distance between surfaces.
 
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  • #33
Highway_Dylan said:
The answer I got is:

## v_0^2=2GM\frac{(D+R)^2}{R(D+2R)(D+3R)}##.

Liable to my own algebraic error of course. I hope that posting this is allowed, since OP showed that he has the intended final answer available.

May I ask how?
 
  • #34
Yalanhar said:
May I ask how?
Try what I (and also others) wrote in post #28. You can get the answer by using conservation of energy.
 
  • #35
Highway_Dylan said:
The answer I got is:

## v_0^2=2GM \frac{(D+R)^2}{R(D+2R)(D+3R)}##
Latex sorted. We're all in agreement then.

@Yalanhar

In any case, if we are taking D to be the distance between the surfaces (which is really odd in a gravitational problem), then I would let ##d = D +3R## be the distance between the centers. Then work with ##d##, as it is simpler and more standard, only converting to D for the final answer.
 

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