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Planned astronomical observatories of the 2020s will be capable of obtainingreflected light photometry and spectroscopy of cool extrasolar giant planets.Here we explain that such data are valuable both for understanding the originand evolution of giant planets as a whole and for preparing for theinterpretation of similar datasets from potentially habitable extrasolarterrestrial planets in the decades to follow.

Imaging Cool Giant Planets in Reflected Light: Science Investigations and Synergy with Habitable Planets