Ejeta, C.; Boehnhardt, H.; Bagnulo, S.; Muinonen, K.; Kolokolova, L.; Tozzi, G. P.: Polarization of Saturn's moon Iapetus. II. Comparison of the dark and the bright sides. Astronomy and Astrophysics 549, A61 (2013)
Ejeta, C.; Muinonen, K.; Boehnhardt, H.; Bagnulo, S.; Kolokolova L.and Guirado, D.; Tozzi, G. P.: Polarization of Saturn's moon Iapetus. III. Models of the bright and the dark sides. Astronomy and Astrophysics 554, A117 (2013)
Ejeta, C.; Boehnhardt, H.; Bagnulo, S.; Tozzi, G. P.: Spectro-polarimetry of the bright side of Saturn's moon Iapetus. Astronomy and Astrophysics 537, A23 (2011)
Various application review phases in 2025. PhD projects in cosmochemistry, planetary science, solar and stellar physics, helioseismology, asteroseismology, ...
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.