Search

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation
Large resolution
Hi-Resolution Export to PDF PPT 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 8.

Top: radius distribution of M dwarf planets in this sample. Middle: [Fe/H] vs. planet radius for the M dwarf planet sample. Bottom: 〈e〉 as a function of the binned planet radius. As G25 showed for planets around FGK stars, we demonstrate an apparent transition in planet occurrence, metallicity, and eccentricity in M dwarf planets.

Other Images in This Article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article

Show More

Copyright and Terms & Conditions

Additional terms of reuse