Here we use a 3-D climate system model to study the habitability of Earth-like planets orbiting in circumbinary systems. In the most extreme cases, Earth-like planets in circumbinary systems could experience variations in the incident stellar flux of up to similar to 50% on similar to 100-day timescales. However, we find that Earth-like planets, having abundant surface liquid water, are generally effective at buffering against these time-dependent changes in the stellar irradiation due to the high thermal inertia of oceans compared with the relatively short periods of circumbinary-driven variations in the received stellar flux. Ocean surface temperatures exhibit little to no variation in time; however, land surfaces can experience modest changes in temperature, thus exhibiting an additional mode of climate variability driven by the circumbinary variations. Still, meaningful oscillations in surface temperatures are only found for circumbinary system architectures featuring the largest physically possible amplitudes in the stellar flux variation. In the most extreme cases, an Earth-like planet could experience circumbinary-driven variations in the global mean land surface temperature of up to similar to 5 K, and variations of local daytime maximum temperatures of up to similar to 12 K on seasonal timescales, while the global mean ocean temperatures vary by less than similar to 2 K. Such seasonal temperature swings over land areas could potentially pose adaptability challenges for extant life. Still, habitable planets in circumbinary systems appear to be remarkably resilient against circumbinary-driven climate variations and can avoid any true climate catastrophes.
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