Associate Professor Kurt Liffman
Kurt Liffman has a B.Sc.(Hons) in Mathematics from the University of Melbourne and PhD in astrophysics from the Department of Physics and Astronomy, Rice University (Houston, TX). Kurt has worked on problems related to the formation of the Solar System at NASA's Johnson Space Center (Houston, TX) and AMES Research Center (Mountain View, CA). Kurt also worked at the CSIRO, where he was affiliated with the astrophysics group at the Australia Telescope National Facility . He currently works at Swinburne as a research scientist and sessional lecturer at SAO. Kurt is also a visiting scientist at the Hawai'i Institute of Geophysics and Planetology. Around two decades ago, Kurt and Michael J. I Brown published a theory suggesting that the some major components found in meteorites (and, possibly, the planets) were formed or reprocessed close to the early Sun and distributed through-out the early Solar System by bipolar jet flows or accretional flows that were produced close to the early Sun in the first few million years of the Solar System. This theory has obtained some preliminary observational confirmation with observations from the Spitzer Space Telescope that show exactly this process occurring in the protostellar systems Ex Lup and HOPS 68. Kurt is currently working with Prof. Sarah Maddison (Swinburne) and the Swinburne planetary science/astrophysics group on projects to better understand how Stellar Systems are formed.
Also published as: Liffman, Kurt; Liffman, K.
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