Particle Shot Tangentially to Surface

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A particle with mass m is shot tangentially to a planet's surface at 3/4 of the escape velocity, leading to a maximum radius from the planet's center before it falls back. The discussion emphasizes the need to apply both conservation of energy and conservation of angular momentum to solve the problem effectively. The particle's trajectory is clarified as elliptical rather than parabolic, indicating it will not achieve orbit. The participant expresses difficulty in starting the solution but acknowledges the importance of using both conservation principles. Ultimately, the conversation revolves around the correct application of physics concepts to determine the particle's maximum distance from the planet.
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Homework Statement


A particle mass m is shot tangentially to the surface of a planet mass M radius R0 at 3/4 escape velocity. Determine the maximum radius the particle achieves from the center of the planet


Homework Equations


Escape Velocity : √(2GM/r)
Energy due to Gravity : -GMm/r2
F=ma
Angular Force : F=mv2/r
Conservation of Angular Momentum : L = r x p or L=mvr



The Attempt at a Solution


Honestly - the beginning of the attempt is where I'm having the issue = I can't decide if I want to use conservation of energy, conservation of angular momentum.

My thought process tells me alright, the particle is shot at a velocity v0 (3/4 escape velocity). This particle has a force acting upon it - the force due to gravity. I can picture exactly what happens to the particle. it won't be shot out fast enough to reach orbit, it reaches a maximum radius r, and then in a parabolic trajectory falls back down to the planet.

Quite honestly - I feel like it should be a very simple solution, I just can't wrap my head around it. Perhaps a tip to start will give me the momentum to find the solution.

Thanks!
 
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trevor51590 said:

Homework Statement


A particle mass m is shot tangentially to the surface of a planet mass M radius R0 at 3/4 escape velocity. Determine the maximum radius the particle achieves from the center of the planet


Homework Equations


Escape Velocity : √(2GM/r)
Energy due to Gravity : -GMm/r2
F=ma
Angular Force : F=mv2/r
Centripetal force, not angular force (whatever that means).
Conservation of Angular Momentum : L = r x p or L=mvr
L=mvr sin θ

The Attempt at a Solution


Honestly - the beginning of the attempt is where I'm having the issue = I can't decide if I want to use conservation of energy, conservation of angular momentum.
You don't need to choose. You have to use both.
My thought process tells me alright, the particle is shot at a velocity v0 (3/4 escape velocity). This particle has a force acting upon it - the force due to gravity. I can picture exactly what happens to the particle. it won't be shot out fast enough to reach orbit, it reaches a maximum radius r, and then in a parabolic trajectory falls back down to the planet.
Elliptical trajectory, not parabolic.
 
Thank you!

I used conservation of energy

1/2mvo2-C/A=1/2mvf2-C/A

For vf I used conservation of angular momentum to put it into terms of vi

Thanks again!
 
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