Particle Shot Tangentially to Surface

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SUMMARY

A particle of mass m is shot tangentially to a planet of mass M and radius R0 at 3/4 of the escape velocity. The maximum radius achieved by the particle from the center of the planet can be determined using both conservation of energy and conservation of angular momentum principles. The escape velocity is calculated as √(2GM/r), while the energy due to gravity is represented as -GMm/r². The particle follows an elliptical trajectory, reaching a maximum radius before falling back to the planet due to gravitational forces.

PREREQUISITES
  • Understanding of escape velocity and its formula: √(2GM/r)
  • Knowledge of gravitational potential energy: -GMm/r²
  • Familiarity with conservation of angular momentum: L = mvr
  • Basic principles of forces and motion (F=ma)
NEXT STEPS
  • Explore the derivation of escape velocity in different gravitational fields.
  • Study the principles of elliptical orbits and their characteristics.
  • Investigate the relationship between kinetic energy and gravitational potential energy in orbital mechanics.
  • Learn about the applications of conservation laws in various physics problems.
USEFUL FOR

Students studying classical mechanics, physics educators, and anyone interested in orbital dynamics and gravitational interactions.

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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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