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Lagrangian for the Kepler Problem

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In a two-body solution ( Kepler Problem) how do you find the Lagrangian, L, if the position vector is:

[tex]x = (v_x * t + x_0, v_y * t + y_0, v_z * t + z_0)[/tex]

Action from Wikipedia is:

[tex]S = \int_{t_1}^{t_2} L * dt [/tex]

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