NDLI: Stability of orbits near large mass ratio binary systems

Content Provider	Springer Nature Link
Author	Bosanac, Natasha Howell, Kathleen C. Fischbach, Ephraim
Copyright Year	2015
Abstract	With improved observational capabilities and techniques, an increasing number of exoplanets have been discovered to orbit in the vicinity of binary star systems. In this investigation, periodic motions near a large mass ratio binary are explored within the context of the circular restricted three-body problem. Specifically, stability analysis is used to explore the effect of the mass ratio on the structure of families of periodic orbits. Such analysis is useful in a variety of applications, including the determination of potentially stable exoplanet motions near a binary star.
Starting Page	27
Ending Page	52
Page Count	26
File Format	PDF
ISSN	09232958
Journal	Celestial Mechanics and Dynamical Astronomy
Volume Number	122
Issue Number	1
e-ISSN	15729478
Language	English
Publisher	Springer Netherlands
Publisher Date	2015-02-18
Publisher Place	Dordrecht
Access Restriction	One Nation One Subscription (ONOS)
Subject Keyword	Circular restricted three-body problem Stability analysis Periodic orbits Binary star systems Pulsar PSR B1620-26 Exoplanets Planets in binaries Bifurcations Astrophysics and Astroparticles Dynamical Systems and Ergodic Theory Aerospace Technology and Astronautics Geophysics/Geodesy Mechanics
Content Type	Text
Resource Type	Article
Subject	Applied Mathematics Mathematical Physics Astronomy and Astrophysics Modeling and Simulation Computational Mathematics Space and Planetary Science

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