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Building planetary systems: linking architectures with formation

Objective

The last few years have seen an explosion in our knowledge of extra-solar planetary systems. However, most exoplanetary systems look nothing like our own: we see “hot Jupiters” which take just days to orbit their parent stars, planets which meander across entire solar systems on highly eccentric orbits, and even planets orbiting twin, binary suns. These planets formed in relatively homogenous discs of cold dust and gas around young, newly-formed stars, but we do not yet understand how this extraordinarily diverse range of planetary architectures was assembled.
BuildingPlanS will establish how the observed architectures of exoplanets link to the physics of their formation. My team will build comprehensive models of the assembly of planetary systems, in order to:
1) understand how systems of giant planets are built.
2) understand the assembly of compact, tightly-packed planetary systems.
3) determine where and when planets form around binary stars.

By focusing on the three main types of known planetary systems we will determine how key physical processes operate in a wide variety of different environments, and build up a detailed understanding of how planetary systems form and evolve. Recently I have played a key role in developing a robust theory of how young, gas-rich protoplanetary discs evolve; this project will establish how these new ideas shape the formation and evolution of planetary systems. My team will consider how forming and newly-formed planets interact with their parent discs, in order to understand the architectures of young planetary systems. We will then follow how these young systems evolve to maturity over billions of years, and test our results against both new observations of planet-forming discs and our ever-growing census of exoplanetary systems. The overall aim of BuildingPlanS is to link exoplanet architectures with their formation and establish a global picture of how planetary systems are built.

Fields of science (EuroSciVoc)

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Programme(s)

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Topic(s)

Calls for proposals are divided into topics. A topic defines a specific subject or area for which applicants can submit proposals. The description of a topic comprises its specific scope and the expected impact of the funded project.

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.

ERC-COG - Consolidator Grant

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Call for proposal

Procedure for inviting applicants to submit project proposals, with the aim of receiving EU funding.

(opens in new window) ERC-2015-CoG

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Host institution

UNIVERSITY OF LEICESTER
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.

€ 1 945 720,96
Address
UNIVERSITY ROAD
LE1 7RH Leicester
United Kingdom

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Region
East Midlands (England) Leicestershire, Rutland and Northamptonshire Leicester
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.

€ 1 945 720,96

Beneficiaries (1)

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