Since the binary separation and mean motion are both one, the Kepler third law givesThe center of mass condition puts the bodies atin the rotating reference frame. Thus the sketch has , , and in that order along the axis, with , andIn the inertial sketch this entire configuration rotates uniformly about .
At a Lagrange point, the test particle is stationary in the rotating reference frame, so . On the axis, makes automatically. The singularities at the two masses split the axis into three intervals, and the balance between gravity and centrifugal acceleration gives one root of in each interval. These are the three Collinear Lagrange points .
For an off-axis equilibrium, . Put . ThenwhileHence and therefore . The two intersections of unit circles centered at and form equilateral triangles with the binary, giving the Triangular Lagrange pointsTogether with the three collinear points, these are the five equilibria of the circular restricted three-body problem.
At , the ordering is . Since ,The equation becomesWriting and retaining first order in and givesConsequentlyThe negative sign says that is slightly less than one binary separation from the dominant mass .
The required Taylor series giveSeek . Substitution in the exact equation from part (iii) gives successivelyThus and , so
Let and be the displacement from the L3 Lagrange point, and put , . The first-order linearization of a dynamical system iswhere every derivative is evaluated at . For the state vector , this becomesThe question's reuse of for the state vector is only notation; its first two entries are the small displacements , not the absolute coordinates.
Write and , so . Sincedirect differentiation givesEvery Collinear Lagrange point has , and in particular
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