compwiz3000
- 17
- 0
If we launch a satellite to a circular orbit around the Earth at height 357.1 km, to find the velocity needed at launch, do we just set the energies equal?:
<br /> - \frac {\mu}{2\left(r_E + h\right)} = \frac {v_L^2}{2} - \frac {\mu}{r_E}<br />
and then solve for v_L?
\mu = GM, where M is the mass of the Earth.
Then, in space, the mechanical energy is
<br /> \frac {v^2}{2} - \frac {\mu}{r}.<br />
Using centripetal force, we have
<br /> \frac {m v^2}{r} = \frac {\mu m}{r^2} \implies v^2 = \frac {\mu}{r},<br />
so the mechanical energy is
<br /> - \frac {\mu}{2r}.<br />
Since the mechanical energy is conserved at the surface, we set it equal to that mechanical energy to find the launch velocity.
<br /> - \frac {\mu}{2\left(r_E + h\right)} = \frac {v_L^2}{2} - \frac {\mu}{r_E}<br />
and then solve for v_L.
Is my reasoning for the launch velocity correct?
<br /> - \frac {\mu}{2\left(r_E + h\right)} = \frac {v_L^2}{2} - \frac {\mu}{r_E}<br />
and then solve for v_L?
\mu = GM, where M is the mass of the Earth.
Then, in space, the mechanical energy is
<br /> \frac {v^2}{2} - \frac {\mu}{r}.<br />
Using centripetal force, we have
<br /> \frac {m v^2}{r} = \frac {\mu m}{r^2} \implies v^2 = \frac {\mu}{r},<br />
so the mechanical energy is
<br /> - \frac {\mu}{2r}.<br />
Since the mechanical energy is conserved at the surface, we set it equal to that mechanical energy to find the launch velocity.
<br /> - \frac {\mu}{2\left(r_E + h\right)} = \frac {v_L^2}{2} - \frac {\mu}{r_E}<br />
and then solve for v_L.
Is my reasoning for the launch velocity correct?
Last edited: