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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 6.

e〉 vs. orbital period for planets within three radius bins: 0.5 < Rp < 1.5R (blue), 1.5 < Rp < 3.5R (green), and 3.5 < Rp < 16R (red). The lines represent the best-fit linear model to each relationship, and the shaded regions represent the 1σ uncertainties. There is no significant relationship present between 〈e〉 and orbital period within any radius bin.

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