133 citations · 1k across the 25 of their papers we have counts for
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Simulations of Water Vapor and Clouds on Rapidly Rotating and Tidally Locked Planets: a 3D Model Intercomparison
Jun Yang, Jeremy Leconte, Eric T. Wolf +4
Robustly modeling the inner edge of the habitable zone is essential for determining the most promising potentially habitable exoplanets for atmospheric characterization. Global cli…
Clouds will likely prevent the detection of water vapor in JWST transmission spectra of terrestrial exoplanets
Thaddeus D. Komacek, Thomas J. Fauchez, Eric T. Wolf +1
We are on the verge of characterizing the atmospheres of terrestrial exoplanets in the habitable zones of M dwarf stars. Due to their large planet-to-star radius ratios and higher…
O2- and CO-Rich Atmospheres for Potentially Habitable Environments on TRAPPIST-1 Planets
Renyu Hu, Luke Peterson, Eric T. Wolf
Small exoplanets of nearby M dwarf stars present the possibility to find and characterize habitable worlds within the next decade. TRAPPIST-1, an ultracool M dwarf star, was recent…
Impact of Clouds and Hazes on the Simulated JWST Transmission Spectra of Habitable Zone Planets in the TRAPPIST-1 System
Thomas J. Fauchez, Martin Turbet, Geronimo L. Villanueva +9
The TRAPPIST-1 system, consisting of an ultra-cool host star having seven known Earth-size planets will be a prime target for atmospheric characterization with JWST. However, the d…
Constraining the magnitude of climate extremes from time-varying instellation on a circumbinary terrestrial planet
Jacob Haqq-Misra, Eric T. Wolf, William F. Welsh +3
Planets that revolve around a binary pair of stars are known as circumbinary planets. The orbital motion of the stars around their center of mass causes a periodic variation in the…
Habitable Zone Boundaries for Circumbinary Planets
Wolf Cukier, Ravi kumar Kopparapu, Stephen R. Kane +4
We use a one-dimensional (1-D) cloud-free climate model to estimate habitable zone (HZ) boundaries for terrestrial planets of masses 0.1 M and 5 M around circumbinary s…