Giant planets: good neighbors for habitable worlds?
arXiv:1804.02183 · doi:10.3847/1538-4357/aaaf72
Abstract
The presence of giant planets influences potentially habitable worlds in numerous ways. Massive celestial neighbors can facilitate the formation of planetary cores and modify the influx of asteroids and comets towards Earth-analogs later on. Furthermore, giant planets can indirectly change the climate of terrestrial worlds by gravitationally altering their orbits. Investigating 147 well characterized exoplanetary systems known to date that host a main sequence star and a giant planet we show that the presence of 'giant neighbors' can reduce a terrestrial planet's chances to remain habitable, even if both planets have stable orbits. In a small fraction of systems, however, giant planets slightly increase the extent of habitable zones provided the terrestrial world has a high climate inertia. In providing constraints on where giant planets cease to affect the habitable zone size in a detrimental fashion, we identify prime targets in the search for habitable worlds.
Published in ApJ,(2018),856,155
References in corpus (18)
- Habitable Zones Around Main-Sequence Stars: Dependence on Planetary Mass
- Kepler constraints on planets near hot Jupiters
- Long-term tidal evolution of short-period planets with companions
- Habitable Climates: The Influence of Eccentricity
- Formation, Habitability, and Detection of Extrasolar Moons
- Gas giant planets as dynamical barriers to inward-migrating super-Earths
- On the formation of terrestrial planets in hot-Jupiter systems
- Habitability of planets on eccentric orbits: the limits of the mean flux approximation
- Jupiter - friend or foe? I: the asteroids
- The Search for other Earths: limits on the giant planet orbits that allow habitable terrestrial planets to form
- Terrestrial Planet Formation in the Presence of Migrating Super-earths
- Effects of variable eccentricity on the climate of an Earth-like world
- Analytic orbit propagation for transiting circumbinary planets
- Stability criteria for hierarchical triple systems
- Survival of habitable planets in unstable planetary systems
- Eccentricity evolution in hierarchical triple systems with eccentric outer binaries
- Stable habitable zones of single Jovian planet systems
- Long term evolution of planetary systems with a terrestrial planet and a giant planet
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- The Fundamental Connections Between the Solar System and Exoplanetary Science
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- System Architecture and Planetary Obliquity: Implications for Long-Term Habitability
- Eta-Earth Revisited II: Deriving a Maximum Number of Earth-like Habitats in the Galactic Disk
- Resilient habitability of nearby exoplanet systems
- Orbital Dynamics and the Evolution of Planetary Habitability in the AU Mic System
- Exploring Climate with Obliquity in a Variable-eccentricity Earth-like World
- On the enlargement of habitable zones around binary stars in hostile environments
- Revised Properties and Dynamical History for the HD 17156 System
- Dynamics and habitability of the TESS circumbinary systems TOI-1338 and TIC-172900988
- New Dynamical State and Habitability of the HD 45364 Planetary System
- Effects of capturing a wide-orbit planet on planetary systems: system stability and Habitable Zone bombardment rates
- Precise Physical Parameters, Habitability, and Orbital Stability of Sun-like SB2 Systems: HD 130669, HD 184467, HD 191854, and HD 214222
- Circumbinary habitable zones in the presence of a giant planet
- Do the planets in the HD 34445 system really exist?