Solving a Satellite Orbit Problem: Help Appreciated!

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A user seeks assistance with a physics problem involving a satellite launched at a 60° angle to the vertical from a point two Earth radii above the North Pole. They initially attempt to calculate the launch velocity using gravitational and centripetal forces but express uncertainty about their approach. Another participant suggests applying conservation of energy principles, noting that the kinetic energy at launch must equal the potential energy at the maximum distance of six Earth radii. The discussion highlights the importance of angular momentum conservation and clarifies the relationship between velocity and radius vector direction at different points in the orbit. The user acknowledges corrections and plans to solve the equations based on the provided guidance.
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Warning read on your own risk: This is my first post here. I'm new to english, sorry for my bad grammar.

Homework Statement


A satellite is launched one time Earth radius straight above the northpole (two times radius from center), with an angle of 60° to vertical.
Find the launch velocity v_{0} so that the satellite won't orbit further away than six times Earth radius from the center of the earth.

Homework Equations


FG=G\frac{Mm}{r^{2}}
FC=m\frac{v^{2}}{r}
FNet=m\cdota

The Attempt at a Solution


I tried solving it by finding the satellite's trajectory.

Initial velocity in x and y direction:
v_{x}=cos 60°\cdotv_{0}
v_{y}=sin 60°\cdotv_{0}

Velocity from gravitational force in x and y direction:
(Θ the angle the satellite makes with the vertical y-axis through the northpole, when it's in orbit)
v_{Gx}=\frac{F_{G} \cdot cos Θ \cdot t}{m}
v_{Gy}=\frac{F_{G} \cdot sin Θ \cdot t}{m}

Total velocity:
(Vector addition)
v_{Tot}=(v_{x} - v_{Gx}) + (v_{y} - v_{Gy})

I don't know if this approach makes sense/ is correct. If it is, how should I continue?
Feel free to ask if something is unclear. Any help or tips are much appreciated.
 
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The position of the satellite and therefore the gravitational force is not constant, that approach does not work.

You will need some conservation laws or (but that is more complicated) solutions to the Kepler problem.
 
What about this solution:
The kinetik energy from the launch must be equal to the potential energy at 6R for the satellite to get no further away than 6R?
U=\frac{-GMm}{R_{2}-R_{1}} and E_{kin}=\frac{mv_{0}^{2}}{2}
The path is not important since it's a conservative field. Energy is conserved.
Therefore
\frac{-GMm}{5R}=\frac{mv_{0}^{2}}{2}
Then I just solve for v_{0}

Is this true?
 
That is better, but still not it. If the potential energy at 6R equals the total energy at 1R, that means the satellite has no kinetic energy, which means it has no velocity. This is possible if the satellite is launched strictly vertically, but it is not in this problem.

You need another conservation law here.
 
The torque is zero because r and F vectors are parallel in a central-force field, therefore the angular momentum is conserved.
Then we have \textbf{r}_{0}\times\textbf{p}_{0}=\textbf{r}_{1}\times\textbf{p}_{1}
I'm not sure if the next steps are correct.
Total energy:
E_{kin0}+E_{pot0}=E_{kin1}+E_{pot1}
\frac{mv^{2}_{0}}{2}+\frac{-GMm}{R}=\frac{mv_{1}^{2}}{2}+\frac{-GMm}{6R}

This is where I think I made a mistake:
v_{0}mr_{0} sin θ = v_{1}mr_{1} sin Θ

In orbit velocity and radius vector are perpendicular
v_{0}m\:1R\:sin (90°+60°) = v_{1}m\:6R\:sin 90°
 
AwesomeTrains said:
The torque is zero because r and F vectors are parallel in a central-force field, therefore the angular momentum is conserved.
Then we have \textbf{r}_{0}\times\textbf{p}_{0}=\textbf{r}_{1}\times\textbf{p}_{1}
I'm not sure if the next steps are correct.
Total energy:
E_{kin0}+E_{pot0}=E_{kin1}+E_{pot1}
\frac{mv^{2}_{0}}{2}+\frac{-GMm}{R}=\frac{mv_{1}^{2}}{2}+\frac{-GMm}{6R}

This is where I think I made a mistake:
v_{0}mr_{0} sin θ = v_{1}mr_{1} sin Θ

All correct so far.

In orbit velocity and radius vector are perpendicular

It is not clear what you mean by that. Is it everywhere in the orbit? Then it is definitely not true, because at the time of launch the angle between the velocity and the radius vector was 60 degrees.

But what about the the farthest point of the orbit? What is the direction of velocity there?
 
voko said:
But what about the the farthest point of the orbit? What is the direction of velocity there?
I meant at 6R the velocity is perpendicular to the radius vector therefore sin is 1.
Then I can solve my equations for initial velocity and velocity at 6R, and I'm done right? :)
(By the way are smileys allowed?)
 
AwesomeTrains said:
I meant at 6R the velocity is perpendicular to the radius vector therefore sin is 1.
Then I can solve my equations for initial velocity and velocity at 6R, and I'm done right? :)

Your reasoning is correct.

I do not understand, however, how you obtained ## \sin (90 + 60) ## for the initial position.

(By the way are smileys allowed?)

Yes. You can use the simple text form like you did, or you can insert graphical smiles. Check out the smiley face icon next too the font controls in the reply box.
 
Okay. Well I thought the angle between the position vector and the initial velocity vector would be 90°+60° because if you put the origo at the center of the earth, and the velocity vector is 60° compared to horizontal.
Made a drawing: http://imageshack.com/a/img838/8807/qyf5.jpg
 
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  • #10
But the problem said "with an angle of 60° to vertical", not horizontal.
 
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  • #11
Oh, oops. Yea it does. Well thanks for the help :biggrin:! Really kind of you
 
  • #12
Please don't include images of that size directly, it does not fit to the page layout. I converted the img-tags to a link.

The position vector points from (0,0) to the satellite, there is no 90° to add.
 
  • #13
Yes, I understand, will solve the equations now and will put in large images as a link in the future.
Thanks for the help :smile:
 
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