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To with 2 and 2EL2 AC2 For Newtonian gravity, we have C Gmim2Part 1: Computeri,T2,Fe, yi, y2 1. Use ra_ z2 + y2 and z-r cos θ to put Equation (1) into Cartesian form. Assume 0 ε < 1, so

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T o 1-ecos θ x = rcos θ 2 when This equation represents an ellipsesetting y = o x= 2x(1-e2) x= 2x(1-e2 ero-ro 0 To 1- e semi major axis a|r (i + e) + r (1-e) 1 a major aXis Now 2 0 1- e2Now setting to compute 0 0 1- e2 1- e2 roe 1- e2 1- e2semi minor axis b=y, 0 1 - e2 minor axis 2ro 1- e2 0

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To with 2 and 2EL2 AC2 For Newtonian gravity, we have C Gmim2 Part 1: Computeri,T2,Fe,...
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