The Department of Earth Sciences is looking for a highly motivated PhD candidate with a MSc background in Earth Sciences, Geochemistry, Geophysics or other appropriate fields. You will work on the project “Geodynamic exploration of emergence and evolution of Hadean paleogeography”, one of several new projects within the PRELIFE programme.
Your jobThe origin of life remains one of the greatest mysteries in science. While many theories have been proposed, no single explanation has yet gained universal agreement. That’s where the
PRELIFE consortium comes in. PRELIFE unites experts across a wide range of disciplines from astronomy, biology, chemistry, computer science, earth and planetary sciences, education, mathematics, to physics. Together we will explore two fundamental questions: How did life emerge on Earth, and how common are the conditions elsewhere in the universe? To answer these profound questions, we will take an interdisciplinary approach, bringing together diverse perspectives to unlock new insights. But we believe this question is not just for scientists, it is for everyone. That’s why we will invite teachers, students, and the public to join us, through educational programs, artistic collaborations, and museum partnerships. We’re searching for answers to life’s biggest questions, and we need your help.
As part of the PRELIFE programme, we offer 15 exciting research projects. Are you a student with deep expertise in your field and a passion for crossing disciplinary boundaries? Each project connects different scientific fields, working together to unlock the secrets of life’s origins and take the public along. Are you in?
Key for the study of the origin and emergence of life on Earth is to estimate what environments were present, and which chemical components, energy sources, and protection to degrading processes were available near and at the surface in the Hadean (4.6-4.0 Ga), for which time interval data are only available from a small number of zircons. Such physical and chemical properties and environments are closely tied to the emergence and evolution of geography: life cannot have existed directly after the Moon-forming impact and the ensuing magma ocean stage, and the rock record shows life had established itself in the Archean (4.0-2.5 Ga) when a solid crust, liquid water oceans, and land existed. The current project aims to evaluate what relief may have existed, and on what timescales, in the course of the Hadean, and, with scenarios for ocean volume on the early Earth, whether land may have existed and what it could have looked like when life emerged.
As a PhD candidate, you will evaluate scenarios through numerical modelling of mantle dynamic and lithosphere (de)formation processes, using the range of possible Hadean compositions and mantle temperature evolution. The project will then evaluate whether and how much land area may have been present given a suite of ocean volume and evolution scenarios, and how long topography may be maintained with a much weaker and hotter crust compared to today. This provides boundary conditions for origin of life, and PRELIFE scenarios.
The study will be carried out by means of forward numerical modelling. Two approaches are envisioned: a simple parameterisation of the required melting laws will be implemented in a proof-of-concept Python code while production runs will ultimately come to rely on the open source community code ASPECT. Model validation includes comparison with the Hadean zircon record.
A personalised training programme will be set up, reflecting your training needs and career objectives. About 20% of your time will be dedicated to this training component, which includes following courses/workshops as well as training on the job in assisting in the Bachelor’s and Master’s programmes of the department at Utrecht University.