|
P45 P51 P73 The Law of Universal Gravitation: FG = GmM/r**2 = mg(r) so that g(r) = GM/r**2
= GMRe**2 / R**2 To stay in orbit, the centripetal force acceleration must balalnce the gravitational force, leading to Vo**2/r = g(r) ------------------------------------------------------------------
(1) where R is the radius of the orbit in units of earth radius. R = 9.8 x Re / Vo**2 The escape speed from the orbit is determined by KE
+ PE(R) = 0 (shown in lecture notes) ----------------------------------------
(3) Vesc = (2 x 9.8 x Re/9.8 x Re / Vo**2)**(1/2) = (2)**0.5 Vo = 2.1 km/s Show that the orbital speed at R = 1 is Vo = 7.9 km/s. P79 |