We know UV radiation isn’t good for us, but can it hold back all forms of life?
Astronomers have been finding planets around M dwarf stars for a while. Can we go even cooler and find planets around the diverse L and T spectral group?
Most Jupiter-like exoplanets go undetected. But do they leave a mark on the more easily detectable inner terrestrial worlds?
The absence of dusty circumplanetary disks around young giant planets suggests moonetesimals grow relatively quickly.
Observations from Hubble and Spitzer bring us one step closer to understanding the atmospheric compositions of intermediate-mass exoplanets.
Interplanetary collisions can explain a number of phenomena in our own solar system — here’s evidence of such a crash shaping the formation of two distant planets. Translate from an Astrobitos bite by Elena Gonzales Egea.