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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 5.

Left: 〈e〉 vs. adjusted planet radius bin centers for the sample of M dwarf singles in this work (red points) and for FGK dwarf singles from G25 (teal points), according to the diagonal binning mechanism described in Section 5.1. 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). Right: same as the left panel, but for multis.

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