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Understanding Exoplanet Atmospheres with UV Observations I: NUV and Blue/Optical

Published onMay 31, 2019
Understanding Exoplanet Atmospheres with UV Observations I: NUV and Blue/Optical
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Abstract

In this white paper we focus on the science case for exoplanet observations at near-UV/blue optical wavelengths. Scattering information encoded in at these wavelengths can distinguish the cause of muted spectral features. These wavelengths also capture atmospheric escape processes, and help characterize mass loss from exoplanet atmospheres.

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