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The Pale Green Dot: A Method to Characterize Proxima Centauri b Using Exo-Aurorae
We examine the feasibility of detecting auroral emission from the potentially habitable exoplanet Proxima Centauri b. Detection of aurorae would yield an independent confirmation of the planet's existence, constrain the presence and composition of its atmosphere, and determine the planet's eccentricity and inclination, thereby breaking the mass-inclination degeneracy. If Proxima Centauri b is a terrestrial world with an Earth-like atmosphere and magnetic field, we estimate the power at thedoi:10.3847/1538-4357/aa6040 fatcat:q6nm4icinrblbijjpfqsgx2dkm