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Tracing the Origins and Evolution of Small Planets using Their Orbital Obliquities

Published onMay 31, 2019
Tracing the Origins and Evolution of Small Planets using Their Orbital Obliquities
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Abstract

We recommend an intensive effort to survey the orbital obliquity distribution of small close-in exoplanets over the coming decade. This is a key tracer of how planets form and migrate. Over the next decade we can observe hundred of planets as small as ~2 REarth, opening a window into the orbital properties of the most common planets.

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