Exploring and understanding
We all know that our world is unique, but we need to understand it in the context of the wider solar system.
If we can understand why Mars has lost so much of its early atmosphere and liquid water, or why Venus’ climate has diverged so markedly from our own, we will be in a better position to take care of our own Earth.
Our researchers are learning about the formation of the solar system, the effects of impact events, and how our magnetosphere shields us from the space environment.
This will allow us to better understand how the solar system evolved, and what is likely to happen in the future.
Researcher profiles and projects
Dr Luke Daly
I co-lead the UK Fireball Network that images fireballs and track meteorites to find out which asteroids they come from and where they land. We recently helped recover the Winchcombe meteorite in 2021.
I use correlative microanalysis to analyse changes that occur in materials in response to space weathering.
By studying water-rich meteorites, Martian meteorites and asteroid sample return mission materials we are uncovering new reservoirs of water in our Solar System and inferring how they evolve and interact on rocky bodies, to help answer the question where did Earth’s oceans come from?
Projects
- Imaging the night sky. The UK Fireball Network takes pictures of the night sky every 30 seconds from six different locations capturing fireballs and also weather, stars, satellites and others
- Correlative microanalysis. Our analytical pipeline can be readily applied to uncover micro-nano-scale structural features of any material from rocks to satellite components
Professor Patrick Harkness
I work on rocket propulsion and surface exploration projects.
Projects
- Rocket test facilities
- Rocket propulsion research
- Surface exploration concepts
- Surface exploration technologies
- Surface exploration projects
Professor Martin Lee
I study carbonaceous chondrites derived from primitive asteroids to explore the earliest history of the Solar System. This work uses an array of microscopy techniques including electron backscatter diffraction (EBSD), X-ray computed tomography (XCT), transmission electron microscopy (TEM), and atom probe tomography (APT). I analyse meteorites that have been recovered from Antarctica, samples that have been returned from primitive asteroids by spacecraft, and meteorites that have fallen recently to Earth including the UK’s very own Winchcombe. I also participate in searches for meteorites that have bene recorded to land in the UK by national fireball camera networks.
I am interested in the earliest history of asteroids and planets – when they were built, what they were made from, and how their constituent rocks and minerals evolved in response to heat, water and pressure. Understanding these processes is key to addressing fundamental questions including how and when Earth became a habitable planet.
Ask me about the Space Nanomaterials Atom Probe. This new analytical facility will enable us to study space materials in an unprecedented level of detail. I will be using it to find drops of liquid water that have preserved for 4500 million years in meteorites derived from primitive asteroids and can provide powerful new insights into the where in the early Solar System the asteroids formed, and how they evolved.
E-mail me at: Martin.Lee@Glasgow.ac.uk, or visit my webpage: Staff - Professor Martin R Lee
Dr Áine O’Brien
I use isotope geochemistry to understand where astrobiologically relevant material originates and how it was processed in the solar system.
Professor Fin Stuart
I measure the trace quantities of gases trapped in primitive meteorites to determine when they were ejected from their parent body and to identify if they preserve remnants of material that pre-dates the formation of the Solar System.
Ask me about new ways to determine how the lunar surface has evolved. We have developed a method using Neon Isotopes produced by Galactic Cosmic Rays to determine how efficiently the upper few metres of lunar soil is gardened by meteroid impacts and electrostatic levitation.
Professor Mark Symes
Applications of electrochemistry in space. For example, oxygen and hydrogen production from water under low gravity and extreme conditions, electrolysis of regoliths for oxygen and metal extraction and development of electrochemical systems for closed chemical cycles (e.g. for life support and resource recycling to support human space exploration).
Dr Kevin Worrall
- Robust Optimal Control using Machine Learning - ESA-funded project considering the application of machine learning for optimal control
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DEEPER - 20m drill for Mars
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OirthirSAT - Academic support for the student-led Cubesat project
Dr Mohammad Yazdani-Asrami
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Superconducting magnets and flux pumps for electric space propulsion.
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Explainable AI and fast predictive models for plasma-thruster performance and optimisation.
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Cryogenic cooling, liquid-hydrogen systems and thermal management.
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Condition monitoring, fault protection and lifetime prediction for electrical and superconducting components.