Spacecraft orbit homework problem

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SUMMARY

The discussion focuses on solving a spacecraft orbit homework problem involving circular and elliptical orbits around Earth. The key equations derived include the circular orbital speed, expressed as v_c = √(gR²/(R+H)), and the speed at perigee for an elliptical orbit, v_0 = √(2gR) [R(1/r - 1/2a)]^(1/2). The eccentricity of the elliptical orbit is also discussed, with the relationship to the parameters R and H. The participant expresses uncertainty regarding the correct formulation of v_0 in terms of R, H, and g, particularly at the perigee where H=0 and r=R.

PREREQUISITES
  • Understanding of gravitational physics, specifically gravitational acceleration (g).
  • Familiarity with orbital mechanics, including concepts of circular and elliptical orbits.
  • Knowledge of energy equations in orbital dynamics.
  • Ability to manipulate algebraic expressions involving variables such as R, H, and eccentricity (e).
NEXT STEPS
  • Study the derivation of orbital speed equations in circular and elliptical orbits.
  • Learn about the conservation of energy in orbital mechanics.
  • Research the concept of eccentricity in elliptical orbits and its implications.
  • Explore practical applications of orbital mechanics in spacecraft design and trajectory planning.
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Students studying physics, particularly those focusing on orbital mechanics, as well as educators looking for examples of gravitational dynamics in homework problems.

kreil
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Homework Statement


Suppose a spacecraft of speed v_c is in a circular orbit around the Earth at a height H from the surface of the earth. The rocket motor is fired in the opposite direction of motion to reduce the satellite's speed to v_0 and make the orbit elliptical. Let R denote the Earth's radius and g the gravitational acceleration on the surface of the earth.

A. Express v_c in terms of R, H, and g.

B. For the spacecraft to land on the Earth surface horizontally at the perigee of the elliptic orbit, find v_0 in terms of R, H, and g. Ignore friction.

C. Express the eccentricity of the elliptic orbit in terms of R and H.

The Attempt at a Solution



For part A I just used the energy equation for a circular orbit, noting r=R+H, k=GMm and g=GM/R^2,

E = T+V=\frac{1}{2}mv_c^2 - \frac{k}{r} = -\frac{k}{2r}

v_c=\left ( \frac{gR^2}{R+H} \right )^{1/2}

For part B, I redid the work from part A for an ellipse, i.e.

E = T+V=\frac{1}{2}mv_0^2 - \frac{k}{r} = -\frac{k}{2a}

v_0 = \sqrt{2gR} \left [ R \left (\frac{1}{r}-\frac{1}{2a} \right ) \right ]^{1/2}

This is where I start having problems. The problem asks for v0 in terms of R, H, and g..but is it not true that when the spacecraft is landing at perigee H=0 and r=R?

The answer I ended up getting for this part came from using r=R=a(1-e) where e is the eccentricity, but I feel shaky about this.

Any thoughts on part B?
 
Last edited:
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This is my opinion.

Point v_0 is the farthest point and
<br /> v_0 \ \bot \ R+H.<br />

The nearest point is R.

So we can conclude that

<br /> 2a=2R+H.<br />
 

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