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

**Authors:** Mark Marley, Nikole Lewis, Giada Arney, Vanessa Bailey, Natasha, Batalha, Charles Beichman, Bj\"orn Benneke, Jasmina Blecic, Kerri Cahoy,, Jeffrey Chilcote, Shawn Domagal-Goldman, Courtney Dressing, Michael, Fitzgerald, Jonathan Fortney, Richard Freedman, Dawn Gelino, John Gizis,, Olivier Guyon, Thomas Greene, Heidi Hammel, Yasuhiro Hasegawa, Nemanja, Jovanovic, Quinn Konopacky, Ravi Kopparapu, Michael Liu, Eric Lopez, Jonathan, Lunine, Roxana Lupu, Bruce Macintosh, Kathleen Mandt, Christian Marois,, Dimitri Mawet, Laura Mayorga, Caroline Morley, Eric Nielsen, Aki Roberge,, Eugene Serabyn, Andrew Skemer, Karl Stapelfeldt, Channon Visscher, Jason Wang

arXiv: 1903.09322 · 2019-03-28

## TL;DR

Upcoming 2020s observatories will enable detailed reflected light studies of cool giant exoplanets, aiding understanding of their evolution and informing future habitable planet research.

## Contribution

This paper highlights the importance of reflected light observations of giant planets for planetary science and future habitable planet exploration.

## Key findings

- Reflected light data help understand giant planet origins.
- Such observations prepare us for studying habitable exoplanets.
- Synergy between giant planet and terrestrial planet studies is emphasized.

## Abstract

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

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Source: https://tomesphere.com/paper/1903.09322