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Bellinger, E. P.; Basu, S.; Hekker, S.; Ball, W.: The Seismic Structures of Solar-Type Stars: Surmising the Speeds of Sound Inside 16 Cygni. KASC10, Birmingham, England (2017)
Guggenberger, E.; Hekker, S.; Basu, S.; Angelou, G. C.; Themessl, N.: Towards an improvement of the scaling relations. The KASC8/TASC1 Workshop Space Asteroseismology: The next generation, Aarhus, Denmark (2015)
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.
The Planetary Plasma Environments group (PPE) has a strong heritage in the exploration of planetary magnetospheres and space plasma interactions throughout the solar system. It has contributed instruments to several past missions that flew-by or orbited Jupiter (Galileo, Cassini, Ulysses). The PPE participates in the JUICE mission by contributing hardware and scientific expertise to the Particle Environment Package (PEP).