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.

Potential supervisors

• Dr Ian Franchi - Senior Research Fellow - Asteroid sample Return missions
• Dr 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

Fees and funding

Please see The Open University website

Qualification and course duration

PhD

MPhil