Spectroscopic monitoring detects phase-locked flares to Proxima d and flare-intensity modulation by Proxima b, producing a -16 G polar field estimate for the inner planet via Poynting-flux modeling.
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The Nautilus Space Observatory white paper outlines four science objectives for tracking planetary evolution timescales, atmospheric mass loss, mean molecular weight and C/O changes, and helium-dominated worlds using proposed high-resolution, broad-wavelength telescope capabilities.
citing papers explorer
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Star-planet interaction in the Proxima system
Spectroscopic monitoring detects phase-locked flares to Proxima d and flare-intensity modulation by Proxima b, producing a -16 G polar field estimate for the inner planet via Poynting-flux modeling.
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Nautilus Space Observatory: The Evolution of Planets and their Atmospheres
The Nautilus Space Observatory white paper outlines four science objectives for tracking planetary evolution timescales, atmospheric mass loss, mean molecular weight and C/O changes, and helium-dominated worlds using proposed high-resolution, broad-wavelength telescope capabilities.