Jansen, C. A.; Burkhardt, C.; Marrocchi, Y.; Schneider, J. M.; Wölfer, E.; Kleine, T.: Condensate evolution in the solar nebula inferred from combined Cr, Ti, and O isotope analyses of amoeboid olivine aggregates. Earth and Planetary Science Letters 627, p. 118567 (2024)
Schneider, J. M.; Burkhardt, C.; Kleine, T.: Distribution of s-, r-, and p-process Nuclides in the Early Solar System Inferred from Sr Isotope Anomalies in Meteorites. The Astrophysical Journal 952, p. L25 (2023)
Windmill, R. J.; Franchi, I. A.; Hellmann, J. L.; Schneider, J. M.; Fridolin, S.; Kleine, T.; Greenwood, R. C.; Anand, M.: Isotopic evidence for pallasite formation by impact mixing of olivine and metal during the first 10 million years of the Solar System. PNAS Nexus 1 (1) (2022)
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).