The giant nature of WD 1856 b implies that transiting rocky planets are rare around white dwarfs

Heat-Flux Limited Cloud Activity and Vertical Mixing in Giant Planet Atmospheres with an Application to Uranus and Neptune

New Mass and Radius Constraints on the LHS 1140 Planets — LHS 1140 b is Either a Temperate Mini-Neptune or a Water World

Tilted circumbinary planetary systems as efficient progenitors of free-floating planets

The positional probability and true host star identification of TESS exoplanet candidates

A roadmap to the efficient and robust characterization of temperate terrestrial planet atmospheres with JWST

A New 2D Energy Balance Model For Simulating the Climates of Rapidly- and Slowly-Rotating Terrestrial Planets

Leave a Reply