Research goal: How do habitable (Earth-like) worlds form and evolve?
My work is principally concerned with the conditions of formation and evolutionary path that have made Earth habitable. The approach I take informs and draws on the insights gained from the chemistries and physical properties of asteroids, planets and moons, dynamical models of Solar System evolution and impact processes, and quests concerning exoplanets and exomoons. As such my work is multi-disciplinary, as are the related thematic volumes and books that I contribute.
Core research is complemented by a range of synergistic activities.
Main research themes:
The first theme, studying meteorites, is my principal area of dedication. The latter two themes address magmatic processes and the deep interior properties of Earth because this information is important for comparison with data from meteorites and lunar materials. Such information provides insight into the origins and behaviours of refractory and volatile element inventories during giant impacts such as that which formed the Moon. These studies also reveal the chemical fingerprint of core formation and late-accretion to the Earth-Moon system. Additionally, the type of work conducted is useful to tracing the mechanisms of continent formation, the rise of plate tectonic processes, and the regulation of (bio)geochemical cycles over Earth history, where their roles are of interest in determining the reasons for habitability and the rise of intelligent life on rocky worlds like our own.
- What does the chemical memory of meteorites and their constituent minerals, tell us about the building blocks for habitable Earth? How do these materials help us to understand and model the history of our Solar System?
- Earth is a planet of our Solar System too, but is it and the array of life that it supports unique in the universe? Are there other worlds teaming with even more life than our own?
- What are the causes and consequences of Large Igneous Province volcanomagmatism over habitable Earth’s history?