Maximum Velocity for Elliptical Orbit

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Homework Help Overview

The problem involves a satellite in a circular orbit at an altitude of 3R around a planet, where the satellite's velocity is altered to create an elliptical orbit. The goal is to determine the maximum factor β by which the velocity can be changed without causing a collision with the planet.

Discussion Character

  • Exploratory, Assumption checking, Mathematical reasoning

Approaches and Questions Raised

  • Participants discuss the conservation of energy in orbital mechanics and the conditions for an elliptical orbit. Some participants question the calculations and assumptions regarding the velocity at the lowest point of the orbit and the factors involved in the energy equations.

Discussion Status

The discussion is ongoing, with participants attempting to clarify their calculations and assumptions. There is a mix of attempts to derive the correct expressions and requests for further elaboration on the calculations presented by others. No consensus has been reached yet.

Contextual Notes

Participants are working under the constraints of homework rules, which may limit the extent of direct assistance. There is also a noted confusion regarding the constants and terms used in the energy equations, indicating potential gaps in understanding the problem setup.

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Homework Statement


A satellite is at an altitude of 3R (R- Radius of the planet) circulating around the planet with a velocity v. In order to make its path elliptical the velocity is changed from v to βv. What should be maximum value of β such that the satellite doesn't collide with the planet?


Homework Equations


First the expression of V is the orbital velocity and
Initial energy = final energy.( in terms of Gravitation)
I can't remember any other equation.

The Attempt at a Solution


I tried but i didn't get the right answer.. The answer is sqrt(2/5)..Thanks in advance for help..
 
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I think you are looking for a minimal value.
Consider the case where the satellite is just "touching" the surface: There are two ways to calculate its velocity, based on two conserved quantities of orbits. They both have to give the same result for a real orbit, this allows to calculate β.
 
Please tell your calculation.. i have also taken the consideration of just touching the surface. .
 
BBAI BBAI said:
Please tell your calculation..
It is your homework problem, not mine. I know how to do it, I don't have to learn that any more.
 
Is the answer coming?
 
I helped you to get the answer yourself.

I tried
If you show your work here, I might look for mistakes.
 
I have done the following things:
0.5mv^2=GMm/4R.
Then 0.5 Mβ^2V^2-GMm/4R=-GmM/R.
What's the mistake here?
 
0.5mv^2=GMm/4R.
Where does this come from? It is wrong by a constant factor.
0.5 Mβ^2V^2-GMm/4R=-GmM/R.
Why do you have M (instead of m) in the first term? Again, where does the "4" come from? What happened to the velocity at the lowest point of the elliptical orbit?
 

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