Skip to main content
SearchLogin or Signup

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
·

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.

The full text of this article is only available in PDF format:



Comments
0
comment

No comments here