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The Evolution of Terrestrial Planets: Insights from Models of Planetary Evolution with Coupled Internal, Atmospheric/Surface Development

Project description

Exploring the evolutionary path of Earth and terrestrial planets

Despite advances in Earth and planetary sciences, understanding of Earth’s evolution is far from complete. While we know that plate tectonics operate on Earth, the timing of onset, length of activity, and initiation mechanisms are still uncertain. This uncertainty is amplified when exploring the evolution of other terrestrial planets. The EU-funded EvoPlans project aims to gain a better understanding of Earth and terrestrial planet evolution, quantifying the processes that affect this evolution, and how these link to control the expression of global tectonics. The goal is to determine the role of coupling between surface, atmosphere, and internal processes in controlling the tectonic and evolutionary history of a planet and address the likelihood of Earth 2.0.

Objective

It is critical to integrate knowledge from multiple disciplines in order to gain a better understanding of the Earth and other terrestrial planets evolution, as well as the effects of this evolution on the expression of surface tectonics. While plate tectonics is currently observed on Earth, both its onset and length of activity are uncertain. Here we will use models of planetary evolution to begin to understand the implications for coupled internal/surface processes through changing lid states over planetary timescales (e.g. C, H2O, and O2, cycles, generation of atmosphere, dynamo generation, and coupled lithosphere-asthenosphere evolution). Further, the internal chemical composition, heterogeneities, and initial conditions within the mantle may be critical factors in setting the evolutionary path of a planet, as such we will determine what role these heterogeneities may play in the evolution of the planet. Finally we seek to understand the controls on the dynamics of a transitional episodic-lid, a state suggested for the early Earth, such as its onset, duration, recurrence interval, and location of overturns, and use these results to assess the implications for planetary development (e.g. dynamo heat flow, generation of atmosphere). This work will begin to address the following open questions: (A) What role does the coupling of internal and surface processes have through changing lid-states? (B) What role do heterogeneities (in viscosity, radiogenics and composition) play in the evolution of the planet? (C) What controls the dynamics of the enigmatic transitional episodic-lid?

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Keywords

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Programme(s)

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Topic(s)

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Funding Scheme

Funding scheme (or “Type of Action”) inside a programme with common features. It specifies: the scope of what is funded; the reimbursement rate; specific evaluation criteria to qualify for funding; and the use of simplified forms of costs like lump sums.

MSCA-IF - Marie Skłodowska-Curie Individual Fellowships (IF)

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Call for proposal

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(opens in new window) H2020-MSCA-IF-2018

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Coordinator

CARDIFF UNIVERSITY
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.

€ 212 933,76
Address
RESEARCH SERVICES C/O MAIN BUILDING
CF10 3AT CARDIFF
United Kingdom

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Region
Wales East Wales Cardiff and Vale of Glamorgan
Activity type
Higher or Secondary Education Establishments
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Total cost

The total costs incurred by this organisation to participate in the project, including direct and indirect costs. This amount is a subset of the overall project budget.

€ 212 933,76
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