Solar system dynamics
by Carl D. Murray · first published 1999
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…larger mass [1]. This means e.g. a typical binary star system would not have stable L4/L5 points. The reference [1] works through this in careful detail and is an excellent reference on this topic. [1] Solar System Dynamics, Murray and Dermott, Cambridge University Press.
on “Lagrange points solved one of physics' biggest problems” ↗…elucidate exoplanet systems. There are plenty of systems discovered by Kepler, CoRoT etc. that require a deep, fundamental understanding of the processes that shape(d) them. [1] http://www.amazon.com/Solar-System-Dynamics-Carl-Murray/dp/0...
on “Interplanetary Transport Network” ↗