Image Details

Choose export citation format:

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 2.

e〉 vs. planet radius bins for the sample of M dwarf planets (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 radius bin (right-hand vertical axis). The median logistic sigmoid model is plotted in dark blue. The 16th and 84th percentiles of the logistic sigmoid are denoted by the dark blue shaded regions.

Other Images in This Article

Show More

Copyright and Terms & Conditions

Additional terms of reuse