Calculating Orbital Distance for a Satellite in Circular Orbit around Mars

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SUMMARY

The discussion centers on calculating the orbital distance for a satellite in a circular orbit around Mars, specifically maintaining a geostationary position above the Martian equator. The key equations used include the gravitational force equation Fc = Fg and the relationship between velocity and orbital radius, leading to the formulation r³ = GM/v². The period of rotation for Mars is established as 8.86 x 10^4 seconds, with the mass of Mars at 6.42 x 10^23 kg and its radius at 3.40 x 10^6 m. The final derived equation for orbital radius is T²/R³ = 4π²/GM.

PREREQUISITES
  • Understanding of gravitational force equations (Fc = Fg)
  • Familiarity with circular motion and orbital mechanics
  • Knowledge of Mars' physical parameters (mass, radius, rotation period)
  • Ability to manipulate algebraic equations for orbital calculations
NEXT STEPS
  • Research the derivation of Kepler's Third Law of planetary motion
  • Explore the implications of geostationary orbits for satellite positioning
  • Learn about the gravitational constant (G) and its application in orbital mechanics
  • Investigate the differences between geostationary and geosynchronous orbits
USEFUL FOR

Aerospace engineers, astrophysicists, and students studying orbital mechanics will benefit from this discussion, particularly those interested in satellite deployment and orbital calculations around celestial bodies like Mars.

Dark_Dragon
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NASA wants to fire a satellite into a circular orbit around Mars that will maintain 'station' above the Martian equator.
what is the distance from the surface of mars?


ok first of all does the term 'station' refer to when g = 0?

and the equation I've used is:
Fc = Fg
mv²/r = GMm/r²

the two 'm' values cancel out and then I am left with:

v²/r = GM/r²

is it then possible to transform the equation into:

r = (GM/r²)*v²

is this procedure correct?
 
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By stationary it means that it will remain at that altitude, not falling or going up at all. Also I think given the context it means that it will be in a geostationary orbit, so it's period is the same as the planets rotational period. (I.e for the earth, it's period would be 24 hours, you'll have to look up the value for mars).

The first step you've used is correct;

\frac{v^2}{r} = \frac{GM}{r^2}

but check the next step...remember you're multiplying by r...not v.

Next can you think of a way of expressing the period of the shuttle in terms of the velocity? (Hint: think of the orbit as a circle, with radius 2pi r, if it's going at speed v, what is the time period T?) You'll have to think of a way of getting that T into the equation above to solve for r.
 
period of rotation of Mars = 8.86 x 10^4 s
mass of Mars = 6.42 x 10^23 kg
Radius of Mars = 3.40 x 10^6 m

if i use v=2πr/T
v = 2*π*3.4e+6 / 8.86e+4
=241.1 m/s

wait, so would my new equation be:
r³ = GM/v² ?

or would i have to go back a few steps and turn it into:
4π²r/T² = GM/r²

if i took that step my equation could then become:
T²/R³ = 4π²/GM
 
Dark_Dragon said:
or would i have to go back a few steps and turn it into:
4π²r/T² = GM/r²

if i took that step my equation could then become:
T²/R³ = 4π²/GM

This is spot on, so now you know the time period, you can find out the radius of its orbit.
 
ok thank you so much for your help =)
 

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