Calculating Kinetic Energy for a Satellite Launch

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SUMMARY

The discussion centers on calculating the kinetic energy of a satellite when it is far from a planet, using principles of physics. The user correctly applied the escape velocity formula, v = √(2GM/r), to determine the minimum kinetic energy required for the satellite to escape the planet's gravitational influence. The final kinetic energy at infinity was derived by subtracting the kinetic energy associated with escape velocity from the initial kinetic energy provided to the satellite. The conversation emphasizes the importance of understanding kinetic and potential energy relationships in gravitational contexts.

PREREQUISITES
  • Understanding of kinetic energy (KE) and potential energy (PE) concepts
  • Familiarity with the escape velocity formula, v = √(2GM/r)
  • Basic knowledge of gravitational forces and their effects on objects
  • Ability to manipulate and rearrange physics equations
NEXT STEPS
  • Study the relationship between kinetic energy and potential energy in gravitational fields
  • Learn about the derivation and implications of escape velocity in different celestial contexts
  • Explore advanced topics in orbital mechanics and energy conservation
  • Practice solving problems involving energy transformations in physics
USEFUL FOR

Students studying physics, particularly those focusing on mechanics and gravitational interactions, as well as educators looking for effective ways to explain energy concepts in celestial dynamics.

alicia.kostka
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Homework Statement



So I just finished a physics test and I'm not sure if I approached a question correctly... Our professor gave us the mass of a satellite, and the mass of an imaginary planet and its radius. Then he gave us the amount of initial kinetic energy given to the satellite when launched. His question was "how much kinetic energy will the satellite have when its very very very far away?" (Assuming no other planet or star is exerting a gravitational force on it)

The Attempt at a Solution



The approach I took was as follows... I used the equation for escape velocity v=\sqrt{}2GM/r ...then using the necessary escape velocity, I used 1/2mv^2 I found the minimum initial kinetic energy for the satellite to escape the planet's orbit. Finally, I subtracted this minimum energy from the actual initial energy given to the satellite to get the final answer.

Does this sound right?
 
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welcome to pf!

hi alicia! welcome to pf! :smile:

(have a square-root: √ and try using the X2 tag just above the Reply box :wink:)

yes, that's correct :smile:

i think you're confused because you're using escape velocity instead of going back to the basics of KE and PE …

escape velocity is the speed (!) ve needed to reach r = ∞ at speed zero

so, since PE is defined as zero, KE + PE = KEr + PEr, ie 0 + 0 = 1/2 mve2 + PEr,

and if v0 > ve, then KE = KEr + PEr = KEr - 1/2 mve2 :wink:
 
Thanks! I think that's ultimately what I did...I ended up subtracting 1/2mve2 from the initial kinetic energy given to the satellite when it was on the surface of the planet. I just didn't do it very elegantly. Sometimes I have to play around with equations before I know what I want to do!
 
hi alicia! :smile:

(just got up :zzz: …)

that's fine … playing around is often a good way of solving things, but (if you have time in the exams) always try to squeeze out the extra couple of marks by making it elegant! :wink:

think "elegant, not elephant!" :biggrin:
 

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