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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