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A New Perspective on the Interiors of Ice-rich Planets: Ice–Rock Mixture Instead of Ice on Top of Rock

The Astrophysical journal, 2022-02, Vol.926 (2), p.150

2022

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Machine-learning Inference of the Interior Structure of Low-mass Exoplanets

The Astrophysical journal, 2020-01, Vol.889 (1), p.42

2020

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A Reanalysis of the Composition of K2-106b: An Ultra-short-period Super-Mercury Candidate

The Astronomical journal, 2023-03, Vol.165 (3), p.97

2023

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Connecting the Gravity Field, Moment of Inertia, and Core Properties in Jupiter through Empirical Structural Models

The Astrophysical journal, 2021-03, Vol.910 (1), p.38

2021

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Waterworlds Probably Do Not Experience Magmatic Outgassing

The Astrophysical journal, 2021-06, Vol.913 (2), p.107

2021

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A Model Earth-sized Planet in the Habitable Zone of α Centauri A/B

The Astrophysical journal, 2022-03, Vol.927 (2), p.134

2022

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Tidally Distorted, Iron-enhanced Exoplanets Closely Orbiting Their Stars

The Astrophysical journal, 2020-05, Vol.894 (1), p.8

2020

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Saturn's Probable Interior: An Exploration of Saturn's Potential Interior Density Structures

The Astrophysical journal, 2020-03, Vol.891 (2), p.109

2020

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Comparison of Machine-learning and Bayesian Inferences for the Interior of Rocky Exoplanets with Large Compositional Diversity

The Astrophysical journal. Supplement series, 2024-06, Vol.272 (2), p.35

2024

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Toward a Self-consistent Evaluation of Gas Dwarf Scenarios for Temperate Sub-Neptunes

The Astrophysical journal, 2024-11, Vol.975 (1), p.101

2024

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Machine-learning Inferences of the Interior Structure of Rocky Exoplanets from Bulk Observational Constraints

The Astrophysical journal. Supplement series, 2023-11, Vol.269 (1), p.1

2023

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Interior Heating of Rocky Exoplanets from Stellar Flares with Application to TRAPPIST-1

Astrophysical journal. Letters, 2022-12, Vol.941 (1), p.L7

2022

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Superadiabaticity in Jupiter and Giant Planet Interiors

Astrophysical journal. Letters, 2021-06, Vol.913 (2), p.L21

2021

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U, Th, and K partitioning between metal, silicate, and sulfide and implications for Mercury's structure, volatile content, and radioactive heat production

The American mineralogist, 2019-09, Vol.104 (9), p.1221-1237

2019

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Random models for exploring planet compositions I: Uranus as an example

Icarus (New York, N.Y. 1962), 2022-08, Vol.382, p.115017, Article 115017

2022

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Onset of convection in internally heated, temperature-dependent, power-law viscosity fluids at large viscosity contrasts

Physics of the earth and planetary interiors, 2023-09, Vol.342, p.107074, Article 107074

2023

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Exploring the tidal responses of ocean worlds with PyALMA

Icarus (New York, N.Y. 1962), 2024-07, Vol.417, p.116120, Article 116120

2024

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How far below the critical Rayleigh number can convection occur in temperature-dependent viscosity fluids?

Physics of the earth and planetary interiors, 2022-08, Vol.329-330, p.106905, Article 106905

2022

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Phase separation in hydrogen-helium mixtures at Mbar pressures

Proceedings of the National Academy of Sciences - PNAS, 2009-02, Vol.106 (5), p.1324-1329

2009

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Can the interior structure influence the habitability of a rocky planet?

Planetary and space science, 2014-08, Vol.98, p.14-29

2014

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The stability of Fe5O6 and Fe4O5 at high pressure and temperature

The American mineralogist, 2019-09, Vol.104 (9), p.1356-1359

2019

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Critique of "Planetary Normal Mode Computation: Parallel Algorithms, Performance, and Reproducibility" by SCC Team From National Tsing Hua University

IEEE transactions on parallel and distributed systems, 2021-11, Vol.32 (11), p.2623-2626

2021

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Titan's Interior Structure and Dynamics After the Cassini-Huygens Mission

Annual review of earth and planetary sciences, 2021-05, Vol.49 (1), p.579-607

2021

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UNDERSTANDING THE MASS-RADIUS RELATION FOR SUB-NEPTUNES: RADIUS AS A PROXY FOR COMPOSITION

The Astrophysical journal, 2014-09, Vol.792 (1), p.1-17

2014

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The Gravitational Imprint of an Interior–Orbital Resonance in Jupiter–Io

The planetary science journal, 2022-04, Vol.3 (4), p.89

2022

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A New Perspective on the Interiors of Ice-rich Planets: Ice–Rock Mixture Instead of Ice on Top of Rock

Machine-learning Inference of the Interior Structure of Low-mass Exoplanets

A Reanalysis of the Composition of K2-106b: An Ultra-short-period Super-Mercury Candidate

Connecting the Gravity Field, Moment of Inertia, and Core Properties in Jupiter through Empirical Structural Models

Waterworlds Probably Do Not Experience Magmatic Outgassing

A Model Earth-sized Planet in the Habitable Zone of α Centauri A/B

Tidally Distorted, Iron-enhanced Exoplanets Closely Orbiting Their Stars

Saturn's Probable Interior: An Exploration of Saturn's Potential Interior Density Structures

Comparison of Machine-learning and Bayesian Inferences for the Interior of Rocky Exoplanets with Large Compositional Diversity

Toward a Self-consistent Evaluation of Gas Dwarf Scenarios for Temperate Sub-Neptunes

Machine-learning Inferences of the Interior Structure of Rocky Exoplanets from Bulk Observational Constraints

Interior Heating of Rocky Exoplanets from Stellar Flares with Application to TRAPPIST-1

Superadiabaticity in Jupiter and Giant Planet Interiors

U, Th, and K partitioning between metal, silicate, and sulfide and implications for Mercury's structure, volatile content, and radioactive heat production

Random models for exploring planet compositions I: Uranus as an example

Onset of convection in internally heated, temperature-dependent, power-law viscosity fluids at large viscosity contrasts

Exploring the tidal responses of ocean worlds with PyALMA

How far below the critical Rayleigh number can convection occur in temperature-dependent viscosity fluids?

Phase separation in hydrogen-helium mixtures at Mbar pressures

Can the interior structure influence the habitability of a rocky planet?

The stability of Fe5O6 and Fe4O5 at high pressure and temperature

Critique of "Planetary Normal Mode Computation: Parallel Algorithms, Performance, and Reproducibility" by SCC Team From National Tsing Hua University

Titan's Interior Structure and Dynamics After the Cassini-Huygens Mission

UNDERSTANDING THE MASS-RADIUS RELATION FOR SUB-NEPTUNES: RADIUS AS A PROXY FOR COMPOSITION

The Gravitational Imprint of an Interior–Orbital Resonance in Jupiter–Io

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