Kossakowski, D.; Kürster, M.; Trifonov, T.; Henning, T.; Kemmer, J.; Caballero, J. A.; Burn, R.; Sabotta, S.; Crouse, J. S.; Fauchez, T. J.et al.; Nagel, E.; Kaminski, A.; Herrero, E.; Rodríguez, E.; González-Álvarez, E.; Quirrenbach, A.; Amado, P. J.; Ribas, I.; Reiners, A.; Aceituno, J.; Béjar, V. J. S.; Baroch, D.; Bastelberger, S. T.; Chaturvedi, P.; Cifuentes, C.; Dreizler, S.; Jeffers, S. V.; Kopparapu, R.; Lafarga, M.; López-González, M. J.; Martín-Ruiz, S.; Montes, D.; Morales, J. C.; Pallé, E.; Pavlov, A.; Pedraz, S.; Perdelwitz, V.; Pérez-Torres, M.; Perger, M.; Reffert, S.; Rodríguez López, C.; Schlecker, M.; Schöfer, P.; Schweitzer, A.; Shan, Y; Shields, A.; Stock, S.; Zapatero Osorio, M. R.; Wolf, E.; Zechmeister, M.: The CARMENES search for exoplanets around M dwarfs. Wolf 1069 b: Earth-mass planet in the habitable zone of a nearby, very low-mass star. Astronomy and Astrophysics 670, p. A84 (2023)
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.