activity
20242026
collaborators

10 papers

astro-ph.EP2026

A Highly Reflective Atmosphere on the Lava World TOI-561b Revealed by JWST/NIRSpec Phase Curve

Samuel Boucher, Lisa Dang, Alex McGinty +15

Ultra-short period (USP) rocky planets are expected to be depleted of any substantial gaseous envelope due to the intense irradiation they receive from their host star, making the…

astro-ph.EP2026

Volatile-rich evolution of molten super-Earth L 98-59 d

Harrison Nicholls, Tim Lichtenberg, Richard D. Chatterjee +3

Small low-density exoplanets are sculpted by strong stellar irradiation, but their primordial compositions and subsequent evolution are still unknown. Two often-considered scenario…

astro-ph.EP2026

Novel Physics of Escaping Secondary Atmospheres May Shape the Cosmic Shoreline

Richard D. Chatterjee, Raymond T. Pierrehumbert

Recent James Webb Space Telescope observations of cool, rocky exoplanets reveal a probable lack of thick atmospheres, suggesting prevalent escape of the secondary atmospheres forme…

astro-ph.EP2025

A Thick Volatile Atmosphere on the Ultrahot Super-Earth TOI-561 b

Johanna K. Teske, Nicole L. Wallack, Anjali A. A. Piette +10

Ultrashort-period (USP) exoplanets -- with R and periods 1 day -- are expected to be stripped of volatile atmospheres by intense host star irradiation…

astro-ph.EP2025

3D Modeling of Moist Convective Inhibition in Idealized Sub-Neptune Atmospheres

Namrah Habib, Raymond T. Pierrehumbert

Atmospheric convection behaves differently in hydrogen-rich atmospheres compared to higher mean molecular weight atmospheres due to compositional gradients of tracers. Previous 1D…

astro-ph.EP2025

Self-limited tidal heating and prolonged magma oceans in the L 98-59 system

Harrison Nicholls, Claire Marie Guimond, Hamish C. F. C. Hay +3

Rocky exoplanets accessible to characterisation often lie on close-in orbits where tidal heating within their interiors is significant, with the L 98-59 planetary system being a pr…