Philidet, J.; Gizon, L.: Interaction of solar inertial modes with turbulent convection. A 2D model for the excitation of linearly stable modes. Astronomy and Astrophysics 673, p. A124 (2023)
The dwarf planet is a bizarre, cryovolcanic world. However, the organic deposits discovered on its surface so far are unlikely to originate from its interior.
The Uranian magnetic field is more expansive than previously thought, according to newly analyzed data from Voyager 2, making it easier to search for moons with oceans.