3.2.32 · D3Orbital Mechanics & Astrodynamics

Worked examples — Three-body problem — restricted (CR3BP), characteristic equation

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Before anything, let us re-anchor four symbols so nothing appears unearned.


The scenario matrix

Every worked example below is tagged with the cell it fills.

Cell Case class Distinguishing feature Example
A Collinear points , generic , → saddle (ALL three) Ex 1 (+ note on ), Ex 8 ()
B Triangular point, small → stable Ex 2
C Triangular point, large → unstable Ex 3
D Degenerate boundary (repeated root) Ex 4
E Limit one primary vanishes Ex 5
F Limit equal masses, most unstable triangular Ex 6
G Real-world word problem pick a real system, decide fate Ex 7 (Sun–Jupiter)
H Exam twist / trap recover the growth rate, not just sign Ex 8 ()

The triangular curvatures are fixed by geometry (parent note): at So for ALL triangular examples: , and And the stability discriminant is , which is the parent's condition. Keep those two facts in view; the triangular examples are all one formula with different .

The figure below is our map for the whole page: its horizontal axis is the mass parameter (running from to , dimensionless), and its vertical axis is the stability discriminant (also dimensionless — a pure number). Where the yellow curve sits above zero (blue shading) triangular points are stable; below zero (pink shading) they are unstable. The pink dotted line marks the critical mass where the curve crosses zero, and each coloured dot marks the of one worked example so you can see where every case lives before we compute it.

Figure — Three-body problem — restricted (CR3BP), characteristic equation
Figure s01 — Triangular-point stability across all : the discriminant curve, the stable/unstable shading, , and the marked example cases.


Worked examples


Recall Self-test (reveal after guessing)

Collinear points are always ::: unstable saddles, because with gives at each of them. Triangular points are stable iff ::: , equivalently . What single quantity decides saddle vs centre for a collinear point? ::: the sign of (product of the -roots). Why don't equal-mass binaries have stable Trojans? ::: , so the discriminant , giving complex and oscillatory runaway. The "4" in the characteristic equation comes from ::: the Coriolis coupling terms squared into the determinant. "One time unit" means ::: one radian of the primaries' orbital angle (the clock where ).

See also: Lagrange points, Jacobi constant & zero-velocity curves, Rotating reference frames — Coriolis & centrifugal forces.