Oscillations in the Habitable Zone around Alpha Centauri B
Duncan Forgan

TL;DR
This study uses latitudinal energy balance models to analyze how Alpha Centauri A influences the habitability and climate oscillations of planets orbiting Alpha Centauri B, revealing temperature variations at habitable zone boundaries.
Contribution
It introduces a novel approach by incorporating Alpha Centauri A's radiative forcing into habitability models for planets around Alpha Centauri B.
Findings
Habitability zone remains largely unchanged by Alpha Centauri A
Temperature oscillations of a few Kelvin are observed at zone boundaries
Climate variability depends on ocean fraction and obliquity
Abstract
The Alpha Centauri AB system is an attractive one for radial velocity observations to detect potential exoplanets. The high metallicity of both Alpha Centauri A and B suggest that they could have possessed circumstellar discs capable of forming planets. As the closest star system to the Sun, with well over a century of accurate astrometric measurements (and Alpha Centauri B exhibiting low chromospheric activity) high precision surveys of Alpha Centauri B's potential exoplanetary system are possible with relatively cheap instrumentation. Authors studying habitability in this system typically adopt habitable zones (HZs) based on global radiative balance models that neglect the radiative perturbations of Alpha Centauri A. We investigate the habitability of planets around Alpha Centauri B using 1D latitudinal energy balance models (LEBMs), which fully incorporate the presence of Alpha…
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