Minimum velocity to throw a object to another planet

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SUMMARY

The discussion centers on calculating the minimum velocity required to throw an object from planet A to planet B, given their respective masses and radii. The key formula derived is v_o = \sqrt \frac{GM(D-R)}{R(3R+D)}, where G is the gravitational constant, M is the mass of the planets, D is the distance between them, and R is the radius of planet A. The analysis emphasizes the importance of integrating the work done by gravitational forces and understanding potential energy in a two-body system. The discussion also highlights the significance of the point x, where gravitational forces are equal, in determining the trajectory of the object.

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  • Familiarity with calculus, specifically integration techniques.
  • Knowledge of Newton's law of gravitation.
  • Ability to apply energy conservation principles in mechanics.
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  • #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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