27 citations · 91 across the 5 of their papers we have counts for
5 papers
Helium Enhanced Planets Along the Upper Edge of the Radius Valley
Isaac Malsky, Leslie Rogers, Eliza M. R. Kempton +1
The low mean densities of sub-Neptunes imply that they formed within a few million years and accreted primordial envelopes. Because these planets receive a total X-ray and extreme…
Where are the Water Worlds?: Self-Consistent Models of Water-Rich Exoplanet Atmospheres
Eliza M. -R. Kempton, Madeline Lessard, Matej Malik +5
It remains to be ascertained whether sub-Neptune exoplanets primarily possess hydrogen-rich atmospheres or whether a population of HO-rich "water worlds" lurks in their midst.…
Internal Structure and CO Reservoirs of Habitable Water-Worlds
Nadejda Marounina, Leslie A. Rogers
Water-worlds are water-rich (>1 wt% HO) exoplanets. The classical models of water-worlds considered layered structures determined by the phase boundaries of pure water. However…
A Statistical Comparative Planetology Approach to Maximize the Scientific Return of Future Exoplanet Characterization Efforts
Jade H. Checlair, Dorian S. Abbot, Robert J. Webber +37
Provided that sufficient resources are deployed, we can look forward to an extraordinary future in which we will characterize potentially habitable planets. Until now, we have had…
Role of the global water ocean on the evolution of Titan's primitive atmosphere
Nadejda Marounina, Olivier Grasset, Gabriel Tobie +1
During the accretion of Titan, impact heating may have been sufficient to allow the global melting of water ice and the release of volatile compounds, mainly constituted of CO2, CH…