Işık, E.; Schmitt, D.; Schüssler, M.: A coupled model of magnetic flux generation and transport in stars. Astron. Nachrichten 328, pp. 1111 - 1113 (2007)
Işık, E.; Schüssler, M.; Solanki, S. K.: Magnetic flux transport on active cool stars and starspot lifetimes. Astronomy and Astrophysics 464, pp. 1049 - 1057 (2007)
Işık, E.; Schüssler, M.; Solanki, S. K.: Magnetic flux transport and the lifetimes of spots on active cool stars. In: Modern Solar Facilities - Advanced Solar Science, pp. 367 - 369 (Eds. Kneer, F.; Puschmann, K. G.; Wittmann, A. D.). Universitätsverlag Göttingen (2007)
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.