# File:Mass parameter vs orbital period ratio circumbinary exoplanets systems.png

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The mass parameter - orbital period ratio relationship for the bi-planet and circumbinary exoplanet systems (dots). The vertical dashed (magenta) line shows the theoretical threshold in $$\mu$$, equal to 0.05. The vertical dotted (cyan) line corresponds to $$\mu = 0.02$$ (from Shevchenko I.I. (2015). Chaotic zones around gravitating binaries, Astrophys. J. 799, 8).

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Date/Time Thumbnail Dimensions User Comment current 13:34, 22 September 2017 881 × 684 (77 KB) José Lages (Talk | contribs) The ''mass parameter - orbital period ratio'' relationship for the bi-planet and circumbinary exoplanet systems (dots). The vertical dashed (magenta) line shows the theoretical threshold in $$\mu$$, equal to 0.05. The vertical dotted (cyan) line corres...

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