Kleine, T.; Mezger, K.; Münker, C.; Palme, H.; Bischoff, A.: 182Hf- 182W isotope systematics of chondrites, eucrites, and martian meteorites: Chronology of core formation and early mantle differentiation in Vesta and Mars. Geochimica et Cosmochimica Acta 68, pp. 2935 - 2946 (2004)
Kleine, T.; Mezger, K.; Palme, H.; Münker, C.: The W isotope evolution of the bulk silicate Earth: constraints on the timing and mechanisms of core formation and accretion. Earth and Planetary Science Letters 228, pp. 109 - 123 (2004)
Münker, C.; Pfänder, J. A.; Weyer, S.; Büchl, A.; Kleine, T.; Mezger, K.: Evolution of Planetary Cores and the Earth-Moon System from Nb/Ta Systematics. Science 301, pp. 84 - 88 (2003)
Kleine, T.; Münker, C.; Mezger, K.; Palme, H.: Rapid accretion and early core formation on asteroids and the terrestrial planets from Hf-W chronometry. Nature 418, pp. 952 - 955 (2002)
Kleine, T.; Budde, G.; Hellmann, J. L.: Tungsten Isotopes and the Origin of Chondrules and Chondrites. In: Chondrules: Records of Protoplanetary Disk Processes, pp. 276 - 299 (Eds. Russell, S. S.; Connolly, H. C.,. J.; Krot, A. N.) (2018)
Kleine, T.; Wadhwa, M.: Chronology of Planetesimal Differentiation. In: Planetesimals: Early Differentiation and Consequences for Planets, pp. 224 - 245 (Eds. Elkins-Tanton, L. T.; Weiss, B. P.) (2017)
Caro, G.; Kleine, T.: Extinct Radionuclides and the Earliest Differentiation of the Earth and Moon. In: Timescale of Magmatic Processes, pp. 9 - 51 (2010)
Kleine, T.: Hafnium—Tungsten Chronometry of Planetary Accretion and Differentiation. In: Chemical Evolution across Space & Time. American Chemical Society (2008)
Halliday, A. N.; Kleine, T.: Meteorites and the Timing, Mechanisms, and Conditions of Terrestrial Planet Accretion and Early Differentiation. In: Meteorites and the Early Solar System II, p. 775 (Eds. Lauretta, D. S.; McSween, H. Y.) (2006)
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).