Celestial Mechanics Flashcards
Newton’s law of gravity
given in exam
Gm1m2
F = ———- . ( r_ / r )
r^2
where r is magnitude of vector r_
Kepler’s first law
Planets move in elliptical orbits with the sun at one focus of the ellipse
Kepler’s second law
The line joining the sun to a planet sweeps out equal area in equal times
(gets faster closer to the focus(sun))
Kepler’s third law
The square of the orbit period t, is proportional to the third power of the semi-major axis of the orbit
t^2 ∝ a^3
General equation for a ellipse
P
r = ——————–
1 + eCosθ
e = 0 is a circle
0
Equation for Kepler’s third law
given in exam
4π^2
t^2 = ———— . a^3
Gm1
What is the Hohmann transfer
when a spacecraft transfers between and LEO to a GEO
What happens during the Hohmann transfer
Two impulse velocities are used. First to take spacecraft out of circular orbit r1, and second to put it into circular orbit r2
What is the equation to find the semi-major axis in a Hohmann transfer
a = (r1 + r2) / 2