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The Orbital Eccentricity–Radius Relation for Planets Orbiting M Dwarfs

  • Authors: Sheila Sagear, Sarah Ballard, Gregory J. Gilbert, Mariangel Albornoz, Christopher Lam

Sheila Sagear et al 2026 The Astronomical Journal 171 .

  • Provider: AAS Journals

Caption: Figure 4.

〈e〉 vs. planet radius bin centers for the sample of M dwarf planets in this work (red points) and for FGK dwarf planets from G25 (teal points). The error bars represent the 16th and 84th percentiles of 〈e〉. The red histogram represents the number of M dwarf planets in each radius bin (right-hand vertical axis).

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