Member Since 1979
Dave J. Stevenson
California Institute of Technology
AGU Research
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Constraints on Europa’s Sub-Surface Ice from Juno Microwave Radiometer Observations
AGU 2024
planetary sciences | 12 december 2024
Steven Levin, Zhimeng Zhang, Scott J. Bolton, Shan...
In September of 2022, the Microwave Radiometer (MWR) on the Juno spacecraft collected 5 minutes of data from within a few hundred km of Europa. The ob...
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The latitudinal dependence of zonal flows depth on Jupiter and Saturn: insights from Juno and Cassini high-degree gravity measurements
AGU 2024
planetary sciences | 12 december 2024
Eli Galanti, Yohai Kaspi, Daniele Durante, Luciano...
The latitudinal profile of the cloud-level winds of Jupiter and Saturn are well observed, showing alternating strong zonal winds in both planets that ...
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Innovative Efficient Mission Concepts for Ice Giant System Exploration: How to Investigate the Origin, Evolution, Rings, Satellites, Deep Atmosphere, Interior Structure and Magnetosphere of Uranus and Neptune
AGU 2024
planetary sciences | 12 december 2024
Scott J. Bolton, Sushil K. Atreya, John E. Connern...
The ice giants are important targets for future exploration as they are distinctively different from gas giants and terrestrial planets. They are most...
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Observations of the Spatial and Power Distributions of Io’s Hotspot-Sourced Heat Flux
AGU 2024
planetary sciences | 11 december 2024
Michael Sowell, David J. Stevenson
The Jovian moon Io is the most volcanically-active body in the Solar System, and these volcanic sources source over half of Io’s total heat flux. Rece...
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A Primordial Venus Moon Might Explain the Planet's Slow Rotation
AGU 2024
planetary sciences | 09 december 2024
Mira Menezes, David J. Stevenson
Earth's slow rotation period (24 hours) arose because of the tidal recession of the Moon.A more typical formation period for large bodies forming from...
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The Fuzzy Cores of Jupiter and Saturn
AGU ADVANCES
04 april 2024
Ravit Helled, David J. Stevenson

New interior models of Jupiter and Saturn suggest that both planets have “fuzzy cores.” These cores should be viewed as central regions...

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Juno Microwave Radiometer Observations of Europa’s and Ganymede’s Subsurface Ice Shell
JUNO’S MULTI-INSTRUMENT VIEW OF EUROPA, GANYMEDE, AND IO II ORAL
planetary sciences | 14 december 2023
Scott J. Bolton, Zhimeng Zhang, Shannon T. Brown, ...
On June 7, 2021, and September 29, 2022, the NASA Juno spacecraft passed Jupiters Galilean moons, Ganymede, and Europa, respectively. The closest appr...
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Europa’s Sub-Surface Ice Observed With The Juno Microwave Radiometer
JUNO’S MULTI-INSTRUMENT VIEW OF EUROPA, GANYMEDE, AND IO I POSTER
planetary sciences | 13 december 2023
Steven Levin, Zhimeng Zhang, Scott J. Bolton, Shan...
Juno flew within 360 km of Europas surface on 29 September, 2022, and the Microwave Radiometer (MWR) mapped part of its ice shell at six frequencies, ...
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