Project Highlights:
Overview:
The STFC Industrial CASE (Cooperative Awards in Science and Technology) studentship provides a 3.5-year stipend that allows the student to spend periods of time on placement at Airbus DS in Stevenage, UK. The cumulative placement period will be no less than 9 months but this will be spread over the period of the studentship and will not normally exceed 18 months.
Protecting the space environment is a critical 21st century challenge to ensure the space sector remains environmentally sustainable and socially responsible. For those that manufacture space and satellite equipment, contamination resulting from surfaces, people and materials is a particular problem that is poorly understood but could have serious adverse impacts on extra-terrestrial environments.
Many materials used in the manufacture of spacecraft, particularly those used for bonding, are silicone-based. This is because they are easy to use, work well in a large range of temperatures, have good adhesion and are UV and ozone resistant. Certain silicones emit low levels of volatile gases. However, in the space environment, there are both thermal and vacuum effects that increase outgassing of certain compounds that can settle on sensitive equipment causing parts, such as lenses, to become contaminated and image quality to be reduced. If they are deposited on equipment that lands on a celestial body, this could contaminate other natural environments, including those that might be habitable.
This studentship builds on a successful Open University/Airbus DS STFC Impact Accelerator Account project (scheme can be found online) and will apply a novel approach to volatile analysis within space sector cleanrooms.
The aims of this studentship are:
Applications should include:
For more details visit the OU Vacancies Page
Applications for this PhD studentship should be sent to STEM-EEES-PHD@open.ac.uk by 12pm (noon) on 29th January 2024
The majority of Venus’ surface consists of basaltic rocks, which are in contact with a hot caustic atmosphere. At these conditions, chemical reactions between the basaltic crust and the atmosphere are expected to alter the venusian surface mineralogy and composition2 . However, without the presence of liquid water, weathering is mostly restricted to oxidation reactions, which are currently not well understood for venusian surface conditions. Better constraints on the alteration mineralogy and the oxidation rate are needed to determine the ages of lava flows and to contribute to the characterisation of the mineralogy and chemistry of the venusian surface such as near infrared (NIR) emissivity spectra, which will be used by the upcoming ESA EnVision and NASA VERITAS (Venus Emissivity, Radio science, InSAR, Topography, And Spectroscopy) missions to map the venusian surface.
This project will use an experimental approach to constrain surface alteration of mafic minerals and basalt under venusian conditions, which is crucial to understand geological processes on Venus including the question whether Venus is still volcanically active. These new constraints on the character and rate of alteration will provide an important new data set in preparation for the upcoming Venus missions.
In detail the project will seek to:
The two sets of simulation experiments and detailed analyses of the samples will be used to determine the alteration products and differences in reaction rates for various starting materials reflecting differences in venusian atmospheric composition.
Applications should include:
Applications for this PhD studentship should be sent to STEM-EEES-PHD@open.ac.uk by 25th January 2024
For more information visit the SPS website: PS5