Kömle, N. I.; Kargl, G.; Thiel, K.; Seiferlin, K.: Thermal properties of cometary ices and sublimation residua including organics. Planetary and Space Science 44, pp. 675 - 689 (1996)
Seiferlin, K.; Kömle, N. I.; Kargl, G.; Spohn, T.: Line heat-source measurements of the thermal conductivity of porous H2O ice, CO2 ice and mineral powders under space conditions. Planetary and Space Science 44, pp. 691 - 704 (1996)
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).