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An Ozone Layer on Early Mars? Leveraging Techniques from Earth Science to Understand Habitability at the Red Planet

Project description

Did Mars once have a protective ozone layer?

In recent years, Mars has attracted increasing interest due to its potential habitability, evidence of past or present life, atmosphere, climate, and other factors. Supported by the Marie Skłodowska-Curie Actions programme, the AREOZONE project will investigate whether Mars once had a protective ozone layer. Such a layer could have shielded surface life from DNA-damaging UV radiation and influenced the planet’s temperature structure and climate. The project will use well-established photochemical models, constrained by observations from complementary missions, build on advances in ozone layer science, and examine the significance of three oxygen isotope ratios. These are key to understanding oxidative chemistry and atmospheric composition changes on Earth.

Objective

For decades, Mars exploration has focused on evidence for life to answer the fundamental question: Are we alone in the universe? I will investigate the possibility of life on early Mars by leveraging decades of research on Earth’s atmosphere to understand that of the red planet. I will use a well-established photochemical model constrained by observations from complementary missions to explore whether ancient Mars ever had a protective ozone layer that could have shielded surface-dwelling life.

The ozone layer is critical on Earth, securing surface habitability from DNA-damaging UV radiation and controlling the temperature structure of the middle atmosphere, with important climatic effects. Our understanding of how Earth’s ozone levels have changed has quickly expanded in recent decades. Here, I will apply lessons learned from Earth to the evolution of a second system—Mars—which will provide unique insights into factors that control planetary atmospheres and the search for life in the universe.

Specifically, I will investigate the utility of ratios of the three oxygen isotopes, used extensively to understand oxidative chemistry and atmospheric composition changes on Earth, to constrain Mars ozone densities through the following three objectives. I will:
1) predict triple oxygen isotope signatures for the present-day Mars atmosphere and compare to observations, to better understand controls on isotope composition;
2) determine realistic palaeo-atmospheric conditions conducive to an ozone layer; and
3) predict the oxygen isotope composition of select geological materials for potential early Mars conditions and prioritise options for future exploration.

We are in the midst of a revolutionary accumulation of spacecraft data and unprecedented Mars exploration, making this work perfectly timed. Preparation for interpretation of measurements from Mars via my proposed modelling is critical to focus future observational efforts from space agencies globally.

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Topic(s)

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HORIZON-TMA-MSCA-PF-EF - HORIZON TMA MSCA Postdoctoral Fellowships - European Fellowships

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Call for proposal

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(opens in new window) HORIZON-MSCA-2024-PF-01

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Coordinator

THE CHANCELLOR, MASTERS AND SCHOLARS OF THE UNIVERSITY OF OXFORD
Net EU contribution

Net EU financial contribution. The sum of money that the participant receives, deducted by the EU contribution to its linked third party. It considers the distribution of the EU financial contribution between direct beneficiaries of the project and other types of participants, like third-party participants.

€ 260 347,92
Address
WELLINGTON SQUARE UNIVERSITY OFFICES
OX1 2JD Oxford
United Kingdom

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Region
South East (England) Berkshire, Buckinghamshire and Oxfordshire Oxfordshire
Activity type
Higher or Secondary Education Establishments
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Total cost

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