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PODCAST SIGNED

Predictions and Observations for Discs: Planetary Cores and dust Aggregates from non-ideal MHD Simulations with radiative Transfer.

Total Cost €

EC-Contrib. €

Partnership

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PODCAST project word cloud

Explore the words cloud of the PODCAST project. It provides you a very rough idea of what is the project "PODCAST" about.

radiation mass compulsory originate grains orders ideal jwst gas grand modern mixtures magnitude poorly question protoplanetary gasgrains planets ska stages couple confront never simulations observations unleashing combining dynamical regions particles holistic first one understand groundbreaking podcast evolution fascinating handle fundamental coupling instruments fragmentation full global flows code cores dynamics micronic dusty disc alma numerical designed astrophysics grow form mhd tremendous dust consistently planet sphere realised physical discs overcome difficulties model

Project "PODCAST" data sheet

The following table provides information about the project.

Coordinator	ECOLE NORMALE SUPERIEURE DE LYON Organization address address: PARVIS RENE DESCARTES 15 city: LYON postcode: 69342 website: n.a. contact info title: n.a. name: n.a. surname: n.a. function: n.a. email: n.a. telephone: n.a. fax: n.a.
Coordinator Country	France [FR]
Total cost	1˙723˙662 €
EC max contribution	1˙723˙662 € (100%)
Programme	1. H2020-EU.1.1. (EXCELLENT SCIENCE - European Research Council (ERC))
Code Call	ERC-2019-COG
Funding Scheme	ERC-COG
Starting year	2020
Duration (year-month-day)	from 2020-02-01 to 2025-01-31

Partnership

Take a look of project's partnership.

#	participants	country	role	EC contrib. [€]
1	ECOLE NORMALE SUPERIEURE DE LYON ECOLE NORMALE SUPERIEURE DE LYON Organization address address: PARVIS RENE DESCARTES 15 city: LYON postcode: 69342 website: n.a. contact info title: n.a. name: n.a. surname: n.a. function: n.a. email: n.a. telephone: n.a. fax: n.a.	FR (LYON)	coordinator	1˙723˙662.00

Map

Project objective

One of the most fascinating and challenging question of Modern Astrophysics is: How do planets form? Indeed, micronic dust grains must grow over 30 orders of magnitude in mass to build planet cores. Global numerical simulations of dust grains that couple the dynamics of the particles to their growth/fragmentation and the radiation in the disc are compulsory to understand this process. Yet, this coupling has never been realised, given tremendous difficulties that originate from fundamental physical properties of dusty flows. The evolution of the dust distribution in protoplanetary discs remains therefore very poorly understood. Our novel groundbreaking code is the first to handle non-ideal MHD, radiation and dust with dynamical growth and fragmentation. We can therefore overcome all past difficulties to model gasgrains mixtures in discs consistently. PODCAST is designed to study the different stages of gas and dust evolution in the various regions of the disc, with the main objective of combining these steps in a holistic model for planet formation. We will confront the results directly with observations, unleashing the full potential of the grand instruments ALMA, SPHERE, JWST and SKA.

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The information about "PODCAST" are provided by the European Opendata Portal: CORDIS opendata.