A super-Earth and two sub-Neptunes transiting the nearby and quiet M dwarf TOI-270
One of the primary goals of exoplanetary science is to detect small, temperate planets passing (transiting) in front of bright and quiet host stars. This enables the characterization of planetary sizes, orbits, bulk compositions, atmospheres and formation histories. These studies are facilitated by small and cool M dwarf host stars. Here we report
Günther, Maximilian N. et al.
Fecha de publicación:
7
2019