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Uranus Pathfinder: exploring the origins and evolution of Ice Giant planets

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Academic year: 2021

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Figure

Fig. 1 Illustration showing the rich variety of science goals for the UP mission: variety of natural satellites, complex ring system, highly asymmetric magnetic field and magnetosphere, atmosphere and interior
Fig. 2 Illustrations showing a a model of Uranus’ interior that is consistent with the gravity and magnetic field data but not with Uranus’ low luminosity (Nettelmann, private communication); b the configuration of Uranus’ internal magnetic field [41]
Fig. 3 Model of Uranus’ interior compared with Uranus’ appearance at multiple wavelengths, sensitive to reflection and scattering of reflected sunlight from uranian clouds and aerosols (first three are short-wavelength images from Voyager 2 (a), HST (b) an
Fig. 4 This composite image of Uranus’ main rings in forward-scattered (left) and back-scattered (right) light shows that a network of dust structures is interleaved among the planet’s dense main rings
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