Comets and Asteroids
Entry requirements
Minimum 2:1 (or equivalent) in a physical science subject
Months of entry
October
Course content
Asteroids and comets are the residual material left from the formation of planets in the inner and outer Solar System respectively. Unlike the planets, many retain material relatively unaltered since their formation 4.6 billion years ago. Their current dynamical and physical properties provide information on their formation and evolution. Our group in the School of Physical Sciences has developed instrumentation for a number of comet missions including Giotto, Stardust and Rosetta, and we are currently involved in the Hayabusa 2 and OSIRIS-REx asteroid sample return missions. We use a range of ground- and space-based telescopes to study the properties of the nuclei and dust production of comets as well as physical properties of asteroids. Our world-leading Advanced Thermophysical Model provides insight into the importance of thermal processes on the physical and dynamical evolution of small asteroids. Laboratory simulations include the evolution of dusty ice cometary analogue surfaces and the effects of impacts on asteroids. Postgraduate students are involved in all aspects of these studies.
- Asteroid regolith production - impacts or thermal cycling?
- Thermal and physical properties of comets - laboratory simulations and Rosetta MUPUS results
- Observations of 67P/Churyumov-Gerasimenko: Linking Rosetta and ground-based results
- Physical and chemical properties of asteroid mission targets
Projects can involve a combination of ground and space-based observations, space mission data analysis, laboratory work, computer modelling or simulation.
- Origin and evolution of comet nuclei
- In-situ measurements of cometary dust
- Physical properties of cometary nucleus analogues for Rosetta
- The shapes of primordial asteroids
- Physics and chemistry of comets & - synthesis of the Rosetta/Philae legacy
Projects currently on offer may be found here.
Potential supervisors
- Dr Ian Franchi - Senior research Fellow - Asteroid sample Return missions
- Professor Simon Green - Professor of Planetary and Space Science - Asteroid and cometary dust observations and mission studies
- Dr Axel Hagermann - Senior lecturer - Laboratory studies of cometary ices and thermal modelling
- Dr Manish Patel - Senior lecturer - Laboratory impact studies
- Dr Ben Rozitis - Royal Astronomical Society Fellow - Asteroid thermal modelling
- Dr Colin Snodgrass - Ernest Rutherford Research Fellow - Comet and asteroid observations
- Professor Ian Wright - Professor of Planetary sciences - Composition and origin of comets
Department specialisms
- Asteroid regolith production - impacts or thermal cycling? - Thermal and physical properties of comets - laboratory simulations and Rosetta MUPUS results - Observations of 67P/Churyumov-Gerasimenko: Linking Rosetta and ground-based results - Physical and chemical properties of asteroid mission targets Projects can involve a combination of ground and space-based observations, space mission data analysis, laboratory work, computer modelling or simulation.
Fees and funding
Please see The Open University website
Qualification and course duration
PhD
MPhil
Course contact details
- Name
- Administrative support
- stem-sps-phd-admin@open.ac.uk
- Phone
- +44 (0)1908 659036