Two Transiting Earth-Size Planets Near Resonance Orbiting a Nearby Cool Star

E. A. Petigura,$^1$ J. E. Schlieder,$^2$ I. J. M. Crossfield,$^3$ et al.

$^1$Caltech, $^2$NASA Ames, $^3$University of Arizona

Motivation & Purpose

An open question is whether small planets are intrinsically more numerous around M dwarfs, or if M dwarf systems are more compact.

This paper can be found in its entirety on the arXiv. Views expressed here are my own and do not necessarily represent those of my institution.