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Detecting Protoplanets and Tracing the Composition and Evolution of Planet-forming Material with Large UV/Optical Observatories

Published onMay 31, 2019
Detecting Protoplanets and Tracing the Composition and Evolution of Planet-forming Material with Large UV/Optical Observatories
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Abstract

This white paper describes how future, large (primary apertures larger than ~12m) UV/optical observatories can detect accreting protoplanets, quantify the evolution of material at planet-forming radii, and provide new constraints on the dispersal of material through disk winds.

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