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The Landscape for Directly Characterizing Potentially Habitable & Inhabited Planets in the Late 2020s and Beyond

Published onSep 30, 2019
The Landscape for Directly Characterizing Potentially Habitable & Inhabited Planets in the Late 2020s and Beyond
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Abstract

We review the landscape for directly characterizing potentially Earth-like planets at UV, optical, and near-IR wavelengths in the late 2020s and beyond. We discuss both ground- and space-based capabilities; ground-based observations are preferred for planets orbiting nearby cool dwarfs, while space is ideal for planets orbiting Sun-like stars.

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