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DOE OSTI · 2519311

Uranus Study Report: KISS

Helled, R. [Univ. of Zurich (Switzerland)]·Millot, M. [Lawrence Livermore National Laboratory (LLNL), Livermore, CA (United States)]
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Abstract

Determining the internal structure of Uranus is a key objective for planetary science. Knowledge of Uranus’s bulk composition and the distribution of elements is crucial to understanding its origin and evolutionary path. In addition, Uranus represents a poorly understood class of “intermediate-mass planets" (intermediate in size between the relatively well studied terrestrial and gas giant planets), which appear to be very common in the Galaxy. As a result, a better characterization of Uranus will also help us to better understand exoplanets in this mass and size regime.

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79 ASTRONOMY AND ASTROPHYSICSAstronomy and AstroPhysics, Physics

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Helled, R. [Univ. of Zurich (Switzerland)], Millot, M. [Lawrence Livermore National Laboratory (LLNL), Livermore, CA (United States)]. 2024-12-04. Uranus Study Report: KISS. https://doi.org/10.2172/2519311

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