David Stevenson

Professor

Caltech

United States

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David Stevenson is a Professor at Caltech in the United States. His research focuses on planetary formation and evolution, with recent articles examining the dynamics of gas giants, particularly Saturn and Jupiter, as well as the interior structures of celestial bodies like Ganymede and Io. His work includes simulations of magnetic fields, crust stability, and the mixing of materials during planetary development.

Articles (13)

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2025

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2024

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2023

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2022

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2022

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2022

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2022

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2022

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2022

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2022

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2021

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2021

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2021

Collaborators (8)

Jeremy Bloxham

Harvard University

UNITED STATES

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Hao Cao

Assistant Professor

University of California, Los Angeles

UNITED STATES

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Yoshinori Miyazaki

California Institute of Technology

UNITED STATES

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Sabine Stanley

Bloomberg Distinguished Professor

Johns Hopkins University

UNITED STATES

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Peter Bodenheimer

Professor Emeriitus

University of California, Santa Cruz

UNITED STATES

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Anton Ermakov

Assistant Professor

Stanford University

UNITED STATES

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M. Zannoni

ITALY

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Ravit Helled

University of Zurich

SWITZERLAND

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David Stevenson

Research Interests

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About

Articles (13)

Formation and Evolution Simulations of Saturn, Including Composition Gradients and Helium Immiscibility

The Stability of a Dense Crust Situated on Small Bodies

Strong Resemblance between Surface and Deep Zonal Winds inside Jupiter Revealed by High-degree Gravity Moments

Dynamo Simulations of Jupiter's Magnetic Field: The Role of Stable Stratification and a Dilute Core

Differential Rotation in Jupiter's Interior Revealed by Simultaneous Inversion for the Magnetic Field and Zonal Flux Velocity

Gravity Field of Ganymede After the Juno Extended Mission

A Subsurface Magma Ocean on Io: Exploring the Steady State of Partially Molten Planetary Bodies

Mixing of Condensable Constituents with H–He during the Formation and Evolution of Jupiter

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

The Lost Meaning of Jupiter’s High-degree Love Numbers

Publisher Correction: Time variation of Jupiter’s internal magnetic field consistent with zonal wind advection

Constraining the Effect of Convective Inhibition on the Thermal Evolution of Uranus and Neptune

Superadiabaticity in Jupiter and Giant Planet Interiors

Collaborators (8)

Jeremy Bloxham

Hao Cao

Yoshinori Miyazaki

Sabine Stanley

Peter Bodenheimer

Anton Ermakov

M. Zannoni

Ravit Helled

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