K2-110 b - a massive mini-Neptune exoplanet

TL;DR

K2-110 b is a massive mini-Neptune exoplanet with well-constrained density, discovered via K2 photometry and RV measurements, offering insights into its composition and atmospheric properties.

Contribution

This study provides one of the most detailed characterizations of a mini-Neptune, combining photometry and RV data to determine its mass, radius, and density.

Findings

K2-110 b has a radius of 2.6 Earth radii and a mass of 16.7 Earth masses.

The planet's density suggests a possible hydrogen atmosphere over an Earth-like interior.

It is unlikely to have lost its atmosphere due to EUV evaporation despite its proximity to the star.

Abstract

We report the discovery of the exoplanet K2-110 b (previously EPIC212521166b) from K2 photometry orbiting in a 13.8637d period around an old, metal-poor K3 dwarf star. With a V-band magnitude of 11.9, K2-110 is particularly amenable to RV follow-up. A joint analysis of K2 photometry and high-precision RVs from 28 HARPS and HARPS-N spectra reveal it to have a radius of 2.6$\pm 0.1 R_{\oplus}$ and a mass of 16.7$\pm 3.2$~M$_{\oplus}$, hence a density of $5.2\pm1.2$ g.cm$^{-3}$, making it one of the most massive planets yet to be found with a sub-Neptune radius. When accounting for compression, the resulting Earth-like density is best fitted by a 0.2 M$_{\oplus}$ hydrogen atmosphere over an 16.5 M$_{\oplus}$ Earth-like interior, although the planet could also have significant water content. At 0.1~AU, even taking into account the old stellar age of $8 \pm 3$ Gyr, the planet is unlikely to have been significantly affected by EUV evaporation. However the planet likely disc-migrated to its current position making the lack of a thick H$_2$ atmosphere puzzling. This analysis has made K2-110 b one of the best-characterised mini-Neptunes with density constrained to less than 30%.