Planetary Dynamics in the α Centauri System: Lyapunov Spectra and Long-term Behaviour
2011 ◽
Vol 7
(S282)
◽
pp. 450-451
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AbstractThe stability of planetary motion in the binary system α Cen A–B is studied. Lyapunov spectra of the motion of the system with a single massive planet are computed on a fine grid of the initial data, and, by means of statistical analysis of the obtained data arrays, chaotic domains are identified in the “pericentric distance — eccentricity” initial data space for the planetary orbit. Association with the initial data domains for the orbits exhibiting close encounters with central stars and for the orbits exhibiting long-term escape is investigated.
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1979 ◽
Vol 42
(04)
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pp. 1135-1140
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2005 ◽
Vol 5
(1)
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pp. 3-50
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2020 ◽
Vol 10
(6)
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pp. 599-609
2018 ◽
Vol 35
(4)
◽
pp. 133-136
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