activity
20242026
collaborators

13 papers

astro-ph.EP2026

Atmospheric diversity of sub-Neptunes from formation with rock, water, and soot

Caroline Dorn, Aaron Werlen, Sean Jordan

Recent JWST detections of CH4 and CO2 in sub-Neptune atmospheres point to a link between atmospheric composition and the nature of planetary building blocks - rock, water, or refra…

astro-ph.EP2026

The Role of Formation Location in Shaping Sulfur-, Nitrogen-, and Carbon-Bearing Species in Super-Earth and Sub-Neptune Atmospheres

Aaron Werlen, Remo Burn, Caroline Dorn +2

Atmospheric compositions of sub-Neptunes and super-Earths are often interpreted as tracers of formation location relative to volatile ice lines. However, prolonged magma oceans can…

astro-ph.EP2026

A New Global Chemical Equilibrium Code: Refractory Element Signatures in Super-Earths and Sub-Neptunes

Simon Grimm, Marie-Luise Steinmeyer, Aaron Werlen +3

The atmospheres of super-Earths and sub-Neptunes can be strongly modified by chemical exchange with their molten interiors during long-lived magma ocean phases. Interpreting atmosp…

astro-ph.EP2026

Oxygen left behind: Atmospheric Enrichment due to Fractionation in Sub-Neptunes using BOREAS

Marilina Valatsou, Caroline Dorn, Pierlou Marty +1

The evolution of exoplanetary atmospheres is strongly influenced by atmospheric escape, particularly for close-in planets. Fractionation during atmospheric loss can preferentially…

astro-ph.EP2026

Coupled Thermal-Chemical Evolution Models of Sub-Neptunes Reveal Atmospheric Signatures of Their Formation Location

Marie-Luise Steinmeyer, Caroline Dorn, Aaron Werlen +1

The observed masses and radii of sub-Neptunes are typically explained by the gas dwarf and the water world scenarios. While their evolutionary history on a population level has bee…

astro-ph.EP2026

Densities of small planets around the M dwarfs TOI-4336 A and TOI-4342 with ESPRESSO: Three sub-Neptunes, one super-Earth, and a Neptune-mass candidate

Léna Parc, Charles Cadieux, Nolan Grieves +27

We present the characterization of two planetary systems orbiting the M dwarfs TOI-4336 A (M3.5V) and TOI-4342 (M0V), each hosting two transiting planets previously validated with…