Overview
About the programme
Planetary Formation and Evolution at The Open University UK uses a variety of cutting-edge laboratory instrumentation to investigate mineralogical, geochemical and isotopic signatures of planetary materials to understand the origin and evolution of their parent bodies.
We are among the leading experts in the world in making high-precision light stable isotope measurements using in-situ techniques, and our Cameca NanoSIMS 50L is currently the only dedicated ion probe facility in the UK for planetary science research.
The planetary samples for our research are allocated through national and international curation facilities as well as through NASA’s Apollo sample collection. Most of our research is carried out in collaboration with planetary scientists, each of whom have an international reputation in their field of expertise.
Results from our projects contribute towards development of future planetary exploration strategy of the European Space Agency such as planning of future sample return missions from the Moon, Mars and other bodies in the Solar System.
Programme Structure
Potential research projects:- Mineralogy/petrology/geochronology of rock samples from differentiated objects (e.g., Moon, Mars, etc.) for understanding planetary formation and evolution
- Comets and meteorites: the volatile inventory of the early Solar System
- Tracking planetary accretion and evolution through stable isotope signatures (e.g., O, Si, Cr)
- Impact effects on isotopic dating systems (e.g. 40Ar/39Ar and U-Th/He)
- Isotope reservoirs in the early solar system
- Origin of organic matter in primitive materials
- Preparation for returned samples (lunar, asteroidal)
- The role of volatiles in the protoplanetary disc. Just how fast are the rapid cooling rates of chondrules
- Physical and chemical properties of matrix in primitive chondrites
- Untangling the earliest stages of planetary differentiation
- Unravelling the secrets of early Solar System processes through laboratory investigations of regolith from a C type asteroid
Key information
Duration
- Full-time
- 36 months
- Part-time
- 72 months
Start dates & application deadlines
- Starting
- Apply before
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- Starting
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- Application period: January to April
Language
Delivered
Disciplines
Astronomy & Space Sciences View 42 other PhDs in Astronomy & Space Sciences in United KingdomAcademic requirements
English requirements
Student insurance
Make sure to cover your health, travel, and stay while studying abroad. Even global coverages can miss important items, so make sure your student insurance ticks all the following:
- Additional medical costs (i.e. dental)
- Repatriation, if something happens to you or your family
- Liability
- Home contents and baggage
- Accidents
- Legal aid
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Other requirements
General requirements
Entry requirements
- Minimum 2:1 undergraduate degree (or equivalent). If you are not a UK citizen, you may need to prove your knowledge of English.
Tuition Fee
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International
15456 GBP/yearTuition FeeBased on the tuition of 15456 GBP per year during 36 months. -
National
4712 GBP/yearTuition FeeBased on the tuition of 4712 GBP per year during 36 months.
Living costs for Milton Keynes
The living costs include the total expenses per month, covering accommodation, public transportation, utilities (electricity, internet), books and groceries.
Funding
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Scholarships Information
Below you will find PhD's scholarship opportunities for Planetary Formation and Evolution.
Available Scholarships
You are eligible to apply for these scholarships but a selection process will still be applied by the provider.
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