In: Physics
What equation describes the motion of planets?
1) Force is a vector having both magnitude and direction.
2) Kepler's laws dictate the motion of planets.
1st Law: distance of planet from the sun is r = p/(1+ecos(theta)) p is semi latus rectum of the ellipse; (r,theta) are polar cordinates. e is the eccentricity of the ellipse.
2nd Law: A line joining a planet and the Sun sweeps out equal areas during equal intervals of time
dA/dt = 0.5 r2 d(theta)/dt
3rd Law: The square of the orbital period of a planet is directly proportional to the cube of the semi-major axis of its orbit.
where
T is the orbital period; M is mass; G is Gravitational constant.