34 citations · 112 across the 6 of their papers we have counts for
6 papers · 1 filter
The nucleosynthetic fingerprint of the outermost protoplanetary disk and early Solar System dynamics
Elishevah van Kooten, Xuchao Zhao, Ian Franchi +6
Knowledge of the nucleosynthetic isotope composition of the outermost protoplanetary disk is critical to understand the formation and early dynamical evolution of the Solar System.…
Anatomy of rocky planets formed by rapid pebble accretion III. Partitioning of volatiles between planetary core, mantle, and atmosphere
Anders Johansen, Thomas Ronnet, Martin Schiller +2
Volatile molecules containing hydrogen, carbon, and nitrogen are key components of planetary atmospheres. In the pebble accretion model for rocky planet formation, these volatile s…
Anatomy of rocky planets formed by rapid pebble accretion II. Differentiation by accretion energy and thermal blanketing
Anders Johansen, Thomas Ronnet, Martin Schiller +2
We explore the heating and differentiation of rocky planets that grow by rapid pebble accretion. Our terrestrial planets grow outside of the ice line and initially accrete 28\% wat…
Anatomy of rocky planets formed by rapid pebble accretion I. How icy pebbles determine the core fraction and FeO contents
Anders Johansen, Thomas Ronnet, Martin Schiller +2
We present a series of papers dedicated to modelling the accretion and differentiation of rocky planets that form by pebble accretion within the lifetime of the protoplanetary disc…
Hybrid accretion of carbonaceous chondrites by radial transport across the Jupiter barrier
Elishevah van Kooten, Martin Schiller, Frederic Moynier +3
Understanding the origin of chondritic components and their accretion pathways is critical to unravel the magnitude of mass transport in the protoplanetary disk, the accretionary h…
A pebble accretion model for the formation of the terrestrial planets in the Solar System
Anders Johansen, Thomas Ronnet, Martin Bizzarro +4
Pebbles of millimeter sizes are abundant in protoplanetary discs around young stars. Chondrules inside primitive meteorites - formed by melting of dust aggregate pebbles or in impa…