Research in planetary and space science (PSS) covers a wide variety of Solar System science and exploration. We investigate the origin and evolution of the Solar System through the physical, geological, chemical and biological processes that drive it. We use laboratory and space mission experiments, remote observation, environmental simulation and modelling to investigate the surfaces and atmospheres of the terrestrial planets, moons, asteroids, comets and extraterrestrial materials.
PSS has a long history of involvement in Solar System exploration through the exploitation of instruments developed at the OU and through international collaborative teams. PSS members are active in the development of new mission proposals and studies with ESA, other space agencies and national programmes. In addition we make use of international ground- and space-based observatories as well as in-house laboratory and simulation facilities. Research students are involved in all aspects of PSS research.
PSS has a long history of involvement in major Solar System exploration missions through the exploitation of instruments developed at the OU, such as on Cassini Huygens, Stardust, Genesis, Rosetta and ExoMars, and through international collaborative teams such as BepiColombo and JUICE. PSS members are active in the development of new mission proposals and studies with ESA, other space agencies and national programmes. In addition we make use of international ground- and space-based observatories in-house laboratory and simulation facilities. Research students are involved in all aspects of PSS research.
Most of our full-time research students are based at our Milton Keynes campus; for details of residence requirements for different modes of study see Full-time study and Part-time study.
Students are equipped with portable laptops (rather than desktop PCs), with enhanced specifications for those needing to run GIS or modelling software.
Our extensive laboratory facilities are broadly subdivided into those used to characterise the chemistry and isotopic composition of matter in the Solar System or the simulation of Earth and Planetary processes. Instruments include state-of-the-art commercially sourced (e.g., NanoSIMS;FIB-SEM; laser Raman microprobe; MS and GC-MS) as well as unique instruments developed in-house (e.g., ‘Finesse’ mass spectrometer; Mars atmosphere and surface simulation chambers; Cometary surface simulation chamber; All-Angle Light Gas Gun). These are backed up by clean rooms and sample preparation facilities, instrument development laboratories and an extensive meteorite collection. Students also have access to analytical facilities across the faculty, as well as the University research computer cluster.
Our PhD graduates have gone on to build successful research careers internationally or applied their skills to industry, the Civil Service or education. You will exit as an accredited scientist with practical, analytical, IT and communication skills appropriate to your field of study, experience of interaction with fellow scientists, and findings published (or ready to publish) in peer-reviewed literature. This can unlock many career paths.