most citedAnatomy of rocky planets formed by rapid pebble accretion I. How icy pebbles determine the core fraction and FeO contents

29 citations · 75 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.EP2026

Coupling dynamical accretion and chemical differentiation: A unified framework for the diversity of Earth and Mars

Zhihui Kong, Beibei Liu, J. ZhangZhou +8

The physical and geochemical differences between Earth and Mars provide fundamental constraints on terrestrial planet formation, yet a self-consistent framework linking dynamical a…

astro-ph.EP2022★ 17 cited

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…

astro-ph.EP2022★ 29 cited

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…

astro-ph.EP2022★ 29 cited

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…