The quadratic first integrals of the torque-free Euler equations for a torque-free rigid body are
Differentiation and substitution of all three Euler equations make each derivative vanish: the coefficients respectively sum to and . At either endpoint these constants are , , proving .
Eliminating the other squared components gives, with ,
Hence and the second Euler equation gives , where increases with . The specified orbit goes from to , so its sign must be negative. The sign in the original PDF's reduced equation is therefore inconsistent with its endpoint conditions. The corrected heteroclinic satisfies
Integrating by separation gives this family for ; the integration constant is a time translation. The printed positive-sign equation instead has the increasing solutions and cannot meet the stated endpoints. For completeness its other real solutions are and the branches on intervals avoiding their pole. These latter branches are excluded by the conserved-energy constraint . The scalar heteroclinic is unique up to translation. For the full angular-velocity vector there are two sign-related branches: simultaneously reversing and preserves all three Euler equations and both endpoints. Full-vector uniqueness therefore also requires choosing one of those branches.

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