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We have developed a comprehensive methodology and an interactive website forcalculating the habitable zone (HZ) of multiple star systems. Using the conceptof spectral weight factor, as introduced in our previous studies of thecalculations of HZ in and around binary star systems, we calculate thecontribution of each star (based on its spectral energy distribution) to thetotal flux received at the top of the atmosphere of an Earth-like planet, anduse the models of the HZ of the Sun to determine the boundaries of the HZ inmultiple star systems. Our interactive website for carrying out thesecalculations is publicly available at http://astro.twam.info/hz . We discussthe details of our methodology and present its application to some of themultiple star systems detected by the Kepler space telescope. We also presentthe instructions for using our interactive website, and demonstrate itscapabilities by calculating the HZ for two interesting analytical solutions ofthe three-body problem.

Calculating the Habitable Zone of Multiple Star Systems (http://astro.twam.info/hz)