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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 3.

Left: 〈e〉 vs. adjusted planet radius radj bin centers for singles with 0.5 < radj < 5.1R⊕ (red points). The red error bars present the 16th and 84th percentiles of 〈e〉. The red histogram represents the number of M dwarf planets in each bin (right-hand vertical axis). Right: same as the left panel, but for multis.

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