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PAMDORA SIGNED

Planetary accretion and migration in discs over all ages

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EC-Contrib. €

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Project "PAMDORA" data sheet

The following table provides information about the project.

Coordinator
MAX-PLANCK-GESELLSCHAFT ZUR FORDERUNG DER WISSENSCHAFTEN EV 

Organization address
address: HOFGARTENSTRASSE 8
city: Munich
postcode: 80539
website: www.mpg.de

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 Germany [DE]
 Total cost 1˙491˙909 €
 EC max contribution 1˙491˙909 € (100%)
 Programme 1. H2020-EU.1.1. (EXCELLENT SCIENCE - European Research Council (ERC))
 Code Call ERC-2017-STG
 Funding Scheme ERC-STG
 Starting year 2018
 Duration (year-month-day) from 2018-01-01   to  2022-12-31

 Partnership

Take a look of project's partnership.

# participants  country  role  EC contrib. [€] 
1    MAX-PLANCK-GESELLSCHAFT ZUR FORDERUNG DER WISSENSCHAFTEN EV DE (Munich) coordinator 1˙491˙909.00

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 Project objective

The goal of this ERC proposal is to make significant progress in our understanding how planetary systems form in protoplanetary discs. In this ambitious research programme I will answer these three key questions:

How does the dust size distribution affect the evolution of ice lines and initial formation location of planetesimals? How do growing planets migrate in protoplanetary discs? How does the disc evolution affect the formation and composition of planetary systems?

I will tackle these questions using a combination of novel ideas and computer simulations in which I will model the three before mentioned connected key stages of planet formation. The disc evolution model will incorporate grain growth and drift with self-consistent temperature structure calculations. The planet migration simulations will map the migration rates from small planets all the way to giant gap opening planets in these discs. Finally, I will combine these topics and compute the assembly of whole planetary systems from multiple small bodies in gas discs to full grown solar systems. Additionally, I will track the chemical composition and evolution of the growing bodies.

These self-consistent models of the formation process from planetary embryos all the way to full planetary systems will be the first of their kind and will shed light on the origin of the variety of planetary systems featuring terrestrial planets, super-Earths, ice and/or gas giants. By incorporating the chemical composition of planets during their formation into my model, I can not only compare the orbital elements to observations, but also their compositions, where observations of the atmospheres of hot Jupiters already exist and future observations of super-Earths will reveal their atmospheric and bulk composition (e.g. through the PLATO space mission), further constraining planet formation theories.

 Publications

year authors and title journal last update
List of publications.
2019 Bertram Bitsch, Sean N. Raymond, Andre Izidoro
Rocky super-Earths or waterworlds: the interplay of planet migration, pebble accretion, and disc evolution
published pages: A109, ISSN: 0004-6361, DOI: 10.1051/0004-6361/201935007
Astronomy & Astrophysics 624 2019-09-04
2019 Trifon Trifonov, Stephan Stock, Thomas Henning, Sabine Reffert, Martin Kürster, Man Hoi Lee, Bertram Bitsch, R. Paul Butler, Steven S. Vogt
Two Jovian Planets around the Giant Star HD 202696: A Growing Population of Packed Massive Planetary Pairs around Massive Stars?
published pages: 93, ISSN: 1538-3881, DOI: 10.3847/1538-3881/aafa11
The Astronomical Journal 157/3 2019-09-04
2018 B Bitsch, R Forsberg, F Liu, A Johansen
Stellar abundance of binary stars: their role in determining the formation location of super-Earths and ice giants
published pages: 3690-3707, ISSN: 0035-8711, DOI: 10.1093/mnras/sty1710
Monthly Notices of the Royal Astronomical Society 479/3 2019-09-04
2019 Bertram Bitsch, Andre Izidoro, Anders Johansen, Sean N. Raymond, Alessandro Morbidelli, Michiel Lambrechts, Seth A. Jacobson
Formation of planetary systems by pebble accretion and migration: growth of gas giants
published pages: A88, ISSN: 0004-6361, DOI: 10.1051/0004-6361/201834489
Astronomy & Astrophysics 623 2019-09-04
2019 S. Pirani, A. Johansen, B. Bitsch, A. J. Mustill, D. Turrini
Consequences of planetary migration on the minor bodies of the early solar system
published pages: A169, ISSN: 0004-6361, DOI: 10.1051/0004-6361/201833713
Astronomy & Astrophysics 623 2019-09-04
2019 Michiel Lambrechts, Alessandro Morbidelli, Seth A. Jacobson, Anders Johansen, Bertram Bitsch, Andre Izidoro, Sean N. Raymond
Formation of planetary systems by pebble accretion and migration
published pages: A83, ISSN: 0004-6361, DOI: 10.1051/0004-6361/201834229
Astronomy & Astrophysics 627 2019-09-02
2018 A. D. Schneider, C. P. Dullemond, B. Bitsch
Surface waves in protoplanetary disks induced by outbursts: Concentric rings in scattered light
published pages: L7, ISSN: 0004-6361, DOI: 10.1051/0004-6361/201833965
Astronomy & Astrophysics 617 2019-09-04
2018 Sean N Raymond, Thibault Boulet, Andre Izidoro, Leandro Esteves, Bertram Bitsch
Migration-driven diversity of super-Earth compositions
published pages: L81-L85, ISSN: 1745-3933, DOI: 10.1093/mnrasl/sly100
Monthly Notices of the Royal Astronomical Society: Letters 479/1 2019-09-04

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