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- W2330921255 abstract "Abstract The growing number of detected planets in binary star systems requires methods for a quick assessment of possible habitability of planets in such environments. We offer an analytic method to determine habitability of a terrestrial planet in binary star systems. In this context we give an answer to the most important question: Do the radiative and gravitational perturbations of a secondary influence the extent of the habitable zone (HZ)? After we have defined the borders of the HZ, we will show the dynamical behaviour of a terrestrial planet in the HZ when adding a Jupiter to the system. In such a system the HZ shows signs of mean motion resonances and secular resonances, depending on the architecture of the planetary system." @default.
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- W2330921255 date "2012-08-01" @default.
- W2330921255 modified "2023-09-23" @default.
- W2330921255 title "On the Habitability of Terrestrial Planets in Binary Star Systems" @default.
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- W2330921255 doi "https://doi.org/10.1017/s1743921313012702" @default.
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