Since the binary separation and mean motion are both one, the Kepler third law gives
The center of mass condition puts the bodies at
in the rotating reference frame. Thus the sketch has , , and in that order along the axis, with , and
In 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 . Then
while
Hence and therefore . The two intersections of unit circles centered at and form equilateral triangles with the binary, giving the Triangular Lagrange points
Together with the three collinear points, these are the five equilibria of the circular restricted three-body problem.
At , the ordering is . Since ,
The equation becomes
Writing and retaining first order in and gives
Consequently
The negative sign says that is slightly less than one binary separation from the dominant mass .
The required Taylor series give
Seek . Substitution in the exact equation from part (iii) gives successively
Thus and , so
Let and be the displacement from the L3 Lagrange point, and put , . The first-order linearization of a dynamical system is
where every derivative is evaluated at . For the state vector , this becomes
The 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 . Since
direct differentiation gives
Every Collinear Lagrange point has , and in particular

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