Cover Image

Vapor equilibrium models of accreting rocky planets demonstrate direct core growth by pebble accretion

Fuente: arXiv

Saved in:

Bibliographic Details
Main Authors:	Steinmeyer, Marie-Luise, Johansen, Anders
Format:	Preprint
Published:	2024
Subjects:	Earth and Planetary Astrophysics
Online Access:	Acceder al recurso
Tags:	Add Tag No Tags, Be the first to tag this record!

Similar Items

Evolution of gas envelopes and outgassed atmospheres of rocky planets formed via pebble accretion
by: Tomberg, Piia Maria, et al.
Published: (2024)

Comment on "Did the terrestrial planets of the Solar System form by pebble accretion?"
by: Johansen, Anders, et al.
Published: (2024)

Exploring the conditions for forming planetesimals by the streaming instability and planetary systems by pebble accretion
by: Johansen, Anders, et al.
Published: (2026)

Did the terrestrial planets of the Solar System form by pebble accretion?
by: Morbidelli, Alessandro, et al.
Published: (2024)

Depletion of moderately volatile elements by pebble accretion in Earth-like planets
by: Olson, Peter L., et al.
Published: (2026)

Reproducing the stellar-mass dependence of the giant planet occurrence rate with pebble accretion models
by: Johnston, Heather F, et al.
Published: (2026)

Giant planet formation via pebble accretion across different stellar masses
by: Shibata, Sho, et al.
Published: (2025)

Influence of migration models and thermal torque on planetary growth in the pebble accretion scenario
by: Saupe, Thomas, et al.
Published: (2020)

Pebble-driven migration of low-mass planets in the 2D regime of pebble accretion
by: Chrenko, O., et al.
Published: (2024)

Formation of wide-orbit giant planets in protoplanetary disks with a decreasing pebble flux
by: Gurrutxaga, Nerea, et al.
Published: (2023)

How planets form by pebble accretion V. Silicate rainout delays contraction of sub-Neptunes
by: Vazan, A., et al.
Published: (2024)

Self-oxidation of the atmospheres of rocky planets with implications for the origin of life
by: Johansen, Anders, et al.
Published: (2024)

Can the giant planets of the Solar System form via pebble accretion in a smooth protoplanetary disc?
by: Lau, Tommy Chi Ho, et al.
Published: (2024)

Formation of flattened planetesimals by gravitational collapse of rotating pebble clouds
by: Lorek, Sebastian, et al.
Published: (2024)

Fast formation of large ice pebbles after FU Orionis outbursts
by: Ros, Katrin, et al.
Published: (2024)

Diversity in planetary architectures from pebble accretion: Water delivery to the habitable zone with pebble snow
by: McCloat, Sean, et al.
Published: (2025)

Formation of cold giant planets around late M dwarfs via core accretion and the fate of inner rocky worlds
by: Sanchez, Mariana, et al.
Published: (2025)

Fundamentals of interior modelling and challenges in the interpretation of observed rocky exoplanets
by: Baumeister, Philipp, et al.
Published: (2025)

Thermal processing of primordial pebbles in evolving protoplanetary disks
by: Colmenares, Maria Jose, et al.
Published: (2024)

Bulk and atmospheric metallicities as direct probes of sequentially varying accretion mechanisms of gas and solids onto planets
by: Hasegawa, Yasuhiro, et al.
Published: (2024)

Formation of multi-planetary systems via pebble accretion in externally photoevaporating discs in stellar clusters
by: Qiao, Lin, et al.
Published: (2026)

A multifluid approach for polydisperse pebble accretion: From particles to fluids, establishing the multifluid framework
by: Konijn, T. J., et al.
Published: (2026)

How leaky? A large parameter study of leaky dust traps to quantify the transport of pebbles and ice in protoplanetary discs
by: Houge, Adrien, et al.
Published: (2026)

A solution for the density dichotomy problem of Kuiper Belt objects with multi-species streaming instability and pebble accretion
by: Cañas, Manuel H., et al.
Published: (2024)

Coupled Thermal-Chemical Evolution Models of Sub-Neptunes Reveal Atmospheric Signatures of Their Formation Location
by: Steinmeyer, Marie-Luise, et al.
Published: (2026)

The effect of dynamic temperatures on pebble dynamics and planet formation
by: Castrejon, Areli, et al.
Published: (2024)

A primordial radius valley as a consequence of planet formation
by: Nielsen, Jesper, et al.
Published: (2025)

Water versus land on temperate rocky planets
by: Guimond, Claire Marie, et al.
Published: (2025)

How the presence of a giant planet affects the outcome of terrestrial planet formation simulations
by: Kong, Zhihui, et al.
Published: (2024)

The evolution of the flux-size relationship in protoplanetary discs by viscous evolution and radial pebble drift
by: Appelgren, Johan, et al.
Published: (2025)

The evolution of catastrophically evaporating rocky planets
by: Curry, Alfred, et al.
Published: (2023)

Simulating the interplay between the snowline pebble flux and ongoing planet formation and migration
by: Astrakhantsev, Danila, et al.
Published: (2026)

The compositions of the HR 8799 planets reflect accretion of both solids and metal-enriched gas
by: Xuan, Jerry W., et al.
Published: (2026)

SPIRou spectropolarimetry of the T Tauri star TW Hydrae: magnetic fields, accretion and planets
by: Donati, J. -F., et al.
Published: (2024)

Wind accretion onto planets orbiting an evolving Solar-like star and their detectability
by: Padilla-López, P., et al.
Published: (2026)

Partial disruption of a planet around a white dwarf: the effect of perturbation from the remnant planet on the accretion
by: Kurban, Abdusattar, et al.
Published: (2024)

UV-processing of icy pebbles in the outer parts of VSI-turbulent disks
by: Flores-Rivera, Lizxandra, et al.
Published: (2024)

The enigmatic dance of the HD 189733A system: Does the planet accrete onto the star?
by: Colombo, Salvatore, et al.
Published: (2024)

Monte Carlo post-processing for radiation hydro simulations of accreting planets in protoplanetary disks
by: Krieger, Anton, et al.
Published: (2025)

Destructuring the disk of AB Aurigae: Dynamics and accretion
by: Boccaletti, Anthony, et al.
Published: (2026)