8.12** (a) By examining the effective potential energy (8.32) find the radius at which a planet...
See problem 8.12 in Classical Mechanics by Taylor 3. Radial Nudges and Oscillations: In your homework, you saw that for the Kepler Problem, circular orbits are stable. If you give the planet a small radial nudge, it oscillates about its original orbit with simple harmonic motion with a period equal to the orbital period. However, after deriving the conic solutions to the Kepler Problem, your professor said that the only possible trajectories are circles, ellipses, parabolas and hyperbolas. a) How...
3) Consider the planet Mercury which has mass 3.34 x1023 kg, radius 2.44x10 m, semimajor axis 5.79x1010 m, and eccentricity .206. a) What is the acceleration due to gravity on the surface of Mercury? b) What is the escape velocity from the surface of Mercury? c) Calculate the force exerted on Mercury by the sun at its perihelion and appihelion. d) What are the perihelion and appihelion velocities of Mercury? e) What is Mercury's angular momentum at these two locations?...