Circumbinary Habitable Zones in the Presence of a Giant Planet

Nikolaos Georgakarakos, Siegfried Eggl, Ian Dobbs-Dixon

Research output: Contribution to journalArticlepeer-review


Determining habitable zones in binary star systems can be a challenging task due to the combination of perturbed planetary orbits and varying stellar irradiation conditions. The concept of “dynamically informed habitable zones” allows us, nevertheless, to make predictions on where to look for habitable worlds in such complex environments. Dynamically informed habitable zones have been used in the past to investigate the habitability of circumstellar planets in binary systems and Earth-like analogs in systems with giant planets. Here, we extend the concept to potentially habitable worlds on circumbinary orbits. We show that habitable zone borders can be found analytically even when another giant planet is present in the system. By applying this methodology to Kepler-16, Kepler-34, Kepler-35, Kepler-38, Kepler-64, Kepler-413, Kepler-453, Kepler-1647, and Kepler-1661 we demonstrate that the presence of the known giant planets in the majority of those systems does not preclude the existence of potentially habitable worlds. Among the investigated systems Kepler-35, Kepler-38, and Kepler-64 currently seem to offer the most benign environment. In contrast, Kepler-16 and Kepler-1647 are unlikely to host habitable worlds.

Original languageEnglish (US)
Article number640830
JournalFrontiers in Astronomy and Space Sciences
StatePublished - Apr 15 2021


  • astrobiology
  • celestial mechanics
  • circumbinary planets
  • habitable planets
  • methods: analytical
  • planet-star interactions

ASJC Scopus subject areas

  • Astronomy and Astrophysics


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