Today’s paper examines the reaction between atmosphere and magma in exoplanets, a key factor in shaping an exoplanet atmosphere
Fabienne Nail writes about how magnetic fields can make modelling atmospheric escape for TRAPPIST-1e and other exoplanets much more difficult.
How much carbon dioxide is too much? Is the habitable zone always habitable? To answer these questions, today’s authors turn up the heat and shove it into overdrive on the highway to the Venus zone!
In order to find life elsewhere in the universe, we need to rule out false positive biosignatures. To get around this, today’s authors use polarized light to distinguish plants from rocks!
How did the Earth keep from freezing over under a faint young Sun 4 billion years ago, and what could it have to do with potatoes and the Moon?!
Could Venus have ever boasted the expansive oceans we find on Earth today? Find out by reading today’s bite about planetary scientists that modeled Venus’s atmosphere!