Rocket Propulsion and Orbital Transfer · USAPhO 2015 #B1

Physics · mechanics

Problem

This problem is divided into three parts. It is possible to solve these three parts independently, but they are not equally weighted. a. An ideal rocket when empty of fuel has a mass mrm_r and will carry a mass of fuel mfm_f. The fuel burns and is ejected with an exhaust speed of vev_e relative to the rocket. The fuel burns at a constant mass rate for a total time TbT_b. Ignore gravity; assume the rocket is far from any other body. i. Determine an equation for the acceleration of the rocket as a function of time t in terms of any or all of t, mfm_f, mrm_r, vev_e, TbT_b, and any relevant fundamental constants. ii. Assuming that the rocket starts from rest, determine the final speed of the rocket in terms of any or all of mrm_r, mfm_f, vev_e, TbT_b, and any relevant fundamental constants. b. The ship starts out in a circular orbit around the sun very near the Earth and has a goal of moving to a circular orbit around the Sun that is very close to Mars. It will make this transfer in an elliptical orbit as shown in bold in the diagram below. This is accomplished with an initial velocity boost near the Earth Δv1\Delta v_1 and then a second velocity boost near Mars Δv2\Delta v_2. Assume that both of these boosts are from instantaneous impulses, and ignore mass changes in the rocket as well as gravitational attraction to either Earth or Mars. Don't ignore the Sun! Assume that the Earth and Mars are both in circular orbits around the Sun of radii RER_E and RM=RE/αR_M = R_E/\alpha respectively. The orbital speeds are vEv_E and vMv_M respectively. [Figure: Orbital diagram showing Earth's orbit at radius RER_E, Mars' orbit at radius RMR_M, and an elliptical transfer orbit (shown in bold) connecting the two circular orbits] i. Derive an expression for the velocity boost Δv1\Delta v_1 to change the orbit from circular to elliptical. Express your answer in terms of vEv_E and α. ii. Derive an expression for the velocity boost Δv2\Delta v_2 to change the orbit from elliptical to circular. Express your answer in terms of vEv_E and α. iii. What is the angular separation between Earth and Mars, as measured from the Sun, at the time of launch so that the rocket will start from Earth and arrive at Mars when it reaches the orbit of Mars? Express your answer in terms of α.

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