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Bifurcation of planetary building blocks during Solar System formation

Science (American Association for the Advancement of Science), 2021-01, Vol.371 (6527), p.365-370

2021

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The effects of short-lived radionuclides and porosity on the early thermo-mechanical evolution of planetesimals

Icarus (New York, N.Y. 1962), 2016-08, Vol.274, p.350-365

2016

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Effect of a single large impact on the coupled atmosphere-interior evolution of Venus

Icarus (New York, N.Y. 1962), 2016-04, Vol.268, p.295-312

2016

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Effect of Water on Lattice Thermal Conductivity of Ringwoodite and Its Implications for the Thermal Evolution of Descending Slabs

Geophysical research letters, 2020-07, Vol.47 (13), p.n/a

2020

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N-body simulations of oligarchic growth of Mars: Implications for Hf–W chronology

Earth and planetary science letters, 2013-03, Vol.366, p.6-16

2013

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Numerical models of the thermomechanical evolution of planetesimals: Application to the acapulcoite-lodranite parent body

Meteoritics & planetary science, 2014-06, Vol.49 (6), p.1083-1099

2014

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Imaging flow focusing and isolation of aqueous fluids in synthetic quartzite: implications for permeability and retained fluid fraction in deep-seated rocks

Progress in earth and planetary science, 2024-12, Vol.11 (1), p.40-16, Article 40

2024

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Combined numerical and experimental study of microstructure and permeability in porous granular media

Solid earth (Göttingen), 2020-06, Vol.11 (3), p.1079-1095

2020

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Origin of the martian dichotomy and Tharsis from a giant impact causing massive magmatism

Icarus (New York, N.Y. 1962), 2011-09, Vol.215 (1), p.346-357

2011

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Pore-scale permeability prediction for Newtonian and non-Newtonian fluids

Solid earth (Göttingen), 2019-10, Vol.10 (5), p.1717-1731

2019

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Impact splash chondrule formation during planetesimal recycling

Icarus (New York, N.Y. 1962), 2018-03, Vol.302, p.27-43

2018

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Olivine aggregates reveal a complex collisional history of the main group pallasite parent body

Meteoritics & planetary science, 2022-05, Vol.57 (5), p.1098-1115

2022

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Scaling laws for the geometry of an impact-induced magma ocean

Earth and planetary science letters, 2021-08, Vol.568, p.116983, Article 116983

2021

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Can Grain Size Reduction Initiate Transform Faults?—Insights From a 3‐D Numerical Study

Tectonics (Washington, D.C.), 2020-10, Vol.39 (10), p.n/a

2020

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A water budget dichotomy of rocky protoplanets from 26Al-heating

Nature astronomy, 2019-02, Vol.3 (4), p.307-313

2019

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The Long-Term Evolution of the Atmosphere of Venus: Processes and Feedback Mechanisms

Space science reviews, 2022-10, Vol.218 (7)

2022

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Modification of icy planetesimals by early thermal evolution and collisions: Constraints for formation time and initial size of comets and small KBOs

Icarus (New York, N.Y. 1962), 2021-07, Vol.363, p.114437, Article 114437

2021

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Mantle fragmentation and incomplete core merging of colliding planetesimals as evidenced by pallasites

Earth and planetary science letters, 2023-09, Vol.617, p.118247, Article 118247

2023

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Magma ascent in planetesimals: Control by grain size

Earth and planetary science letters, 2019-02, Vol.507, p.154-165

2019

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Protocore destabilization in planetary embryos formed by cold accretion: Feedbacks from non-Newtonian rheology and energy dissipation

Icarus (New York, N.Y. 1962), 2011-05, Vol.213 (1), p.24-42

2011

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Olivine grain growth in partially molten Fe–Ni–S: A proxy for the genesis of pallasite meteorites

Earth and planetary science letters, 2018-12, Vol.504, p.38-52

2018

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Numerical modeling of protocore destabilization during planetary accretion: Methodology and results

Icarus (New York, N.Y. 1962), 2009-12, Vol.204 (2), p.732-748

2009

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Combined impact and interior evolution models in three dimensions indicate a southern impact origin of the Martian Dichotomy

Icarus (New York, N.Y. 1962), 2024-09, Vol.420, p.116137, Article 116137

2024

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Investigating the feasibility of an impact-induced Martian Dichotomy

Icarus (New York, N.Y. 1962), 2023-03, Vol.392, p.115395, Article 115395

2023

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Mars's Crustal and Volcanic Structure Explained by Southern Giant Impact and Resulting Mantle Depletion

Geophysical research letters, 2024-03, Vol.51 (6), p.n/a

2024

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Bifurcation of planetary building blocks during Solar System formation

The effects of short-lived radionuclides and porosity on the early thermo-mechanical evolution of planetesimals

Effect of a single large impact on the coupled atmosphere-interior evolution of Venus

Effect of Water on Lattice Thermal Conductivity of Ringwoodite and Its Implications for the Thermal Evolution of Descending Slabs

N-body simulations of oligarchic growth of Mars: Implications for Hf–W chronology

Numerical models of the thermomechanical evolution of planetesimals: Application to the acapulcoite-lodranite parent body

Imaging flow focusing and isolation of aqueous fluids in synthetic quartzite: implications for permeability and retained fluid fraction in deep-seated rocks

Combined numerical and experimental study of microstructure and permeability in porous granular media

Origin of the martian dichotomy and Tharsis from a giant impact causing massive magmatism

Pore-scale permeability prediction for Newtonian and non-Newtonian fluids

Impact splash chondrule formation during planetesimal recycling

Olivine aggregates reveal a complex collisional history of the main group pallasite parent body

Scaling laws for the geometry of an impact-induced magma ocean

Can Grain Size Reduction Initiate Transform Faults?—Insights From a 3‐D Numerical Study

A water budget dichotomy of rocky protoplanets from 26Al-heating

The Long-Term Evolution of the Atmosphere of Venus: Processes and Feedback Mechanisms

Modification of icy planetesimals by early thermal evolution and collisions: Constraints for formation time and initial size of comets and small KBOs

Mantle fragmentation and incomplete core merging of colliding planetesimals as evidenced by pallasites

Magma ascent in planetesimals: Control by grain size

Protocore destabilization in planetary embryos formed by cold accretion: Feedbacks from non-Newtonian rheology and energy dissipation

Olivine grain growth in partially molten Fe–Ni–S: A proxy for the genesis of pallasite meteorites

Numerical modeling of protocore destabilization during planetary accretion: Methodology and results

Combined impact and interior evolution models in three dimensions indicate a southern impact origin of the Martian Dichotomy

Investigating the feasibility of an impact-induced Martian Dichotomy

Mars's Crustal and Volcanic Structure Explained by Southern Giant Impact and Resulting Mantle Depletion

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