
TEMPEST thermophysical model
- Surface roughness, multiple heat-conduction schemes and modular scattering
- Validated against the established Spencer 1D thermal model
- Applied to Lucy, Europa, Enceladus, Lunar Trailblazer and the PRIME mission concept
I’m a planetary scientist in the final year of a DPhil in Atmospheric, Oceanic and Planetary Physics at the University of Oxford, supervised by Dr Carly Howett. I specialise in thermal-infrared remote sensing: using temperature measurements from spacecraft to work out what planetary surfaces are made of and what might be happening beneath them.
I lead development of TEMPEST, an open-source thermophysical model, and I’m a member of the Surface Composition Working Group for NASA’s Lucy mission. Alongside modelling, I work on infrared imaging and thermal mapping instruments, from filter design for Oxford’s Enceladus Thermal Mapper to preparing for Europa Clipper, JUICE and a future ESA mission to Enceladus.
Before Oxford I worked as an acoustics consultant and as a technical officer at UNSW Sydney, and founded a surfboard company. I’m now looking for postdoctoral positions in planetary science, and I’m open to consulting work on infrared imaging, thermal mapping and instrument design.
DPhil Atmospheric, Oceanic & Planetary Physics
University of Oxford
MPhys Physics (First Class)
University of Exeter (exchange year at University of Wollongong, Australia)
I build and apply thermal models that turn spacecraft measurements into physical understanding of planetary surfaces, from binary asteroids to the icy shells of ocean worlds.

With Carly Howett at the Donaldjohanson encounter, Boulder, 2025

I’m always happy to talk about thermophysical modelling, missions to icy moons, collaborations, postdoctoral opportunities or consulting on infrared imaging and thermal mapping. Send me a message here or email me directly.