Question

formula of state keplers law of planetary motion ​

Answer 1

Explanation:

In Satellite Orbits and Energy, we derived Kepler's third law for the special case of a circular orbit. Equation 13.8 gives us the period of a circular orbit of radius r about Earth: T=2π√r3GME. For an ellipse, recall that the semi-major axis is one-half the sum of the perihelion and the aphelion.

Answer 2

Answer:

vvhksufdtidtitkysti

Explanation:

ysbsjdbsk sisbsis sjdbhqvwbwbwvw