Our M-dwarf Models Just Aren’t Good Enough
We need to know the radii of M-dwarfs to study their exoplanets, and the models aren’t much help.
We need to know the radii of M-dwarfs to study their exoplanets, and the models aren’t much help.
Are planets just as likely to form around binary stars as they are around single stars? Today’s authors are asking this very question.
Nearby Super-Jupiters with very tight orbits produce gravitational waves that will be detectable by space-based gravitational wave detectors.
Today’s authors search for Jupiter analogs in foreign star systems to see how these giant worlds might affect the development of planets closer to the sun.
Higher-order effects are beginning to surface in the photometry of exoplanets. Today we look at the way particles can add a ring to an exoplanet’s silhouette.
An novel method that could add texture to other worlds.