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NASA NTRS · 20140002071

The Formation Environment of Jupiter's Moons

Turner, Neal·Lee, Man Hoi·Sano, Takayoshi
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Abstract

Do circumjovian disk models have conductivities consistent with the assumed accretion stresses? Broadly, YES, for both minimum-mass and gas-starved models: magnetic stresses are weak in the MM models, as needed to keep the material in place. Stresses are stronger in the gas-starved models, as assumed in deriving the flow to the planet. However, future minimum-mass modeling may need to consider the loss of dust-depleted gas from the surface layers to the planet. The gas-starved models should have stress varying in radius. Dust evolution is a key process for further study, since the recombination occurs on the grains.

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Turner, Neal, Lee, Man Hoi, Sano, Takayoshi. 2012-06-25. The Formation Environment of Jupiter's Moons. https://ntrs.nasa.gov/citations/20140002071

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