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Cassini-Huygens

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Cassini at Saturn

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Abstract

The Saturnian system was visited by robotic explorers from the planet Earth in three successive years: 1979, 1980 and 1981. In contrast to the expected bland frozen realm, the system has turned out to be incredibly rich in diversity: Enceladus has been comprehensively resurfaced, and might still be undergoing cryovolcanic activity with geysers venting jets of water into space; Titan has a dense reducing atmosphere that may well be in a prebiotic state; Iapetus has its enigmatic dark hemisphere; and Phoebe is almost certainly a captured comet or asteroid - maybe even an object that strayed in from the Kuiper Belt. It was inevitable, therefore, that within a few years planning would get underway to dispatch a follow-up mission. As in the case of the Galileo mission to Jupiter, the next spacecraft to Saturn would enter orbit to conduct an in-depth study. In 1982, a Joint Working Group of the US National Academy of Sciences and the European Science Foundation recommended a‘Saturn Orbiter and Titan Probe’. The following year, NASA’s Solar System Exploration Committee, in recognising Titan’s uniqueness, assigned its top priority in the outer Solar System to a‘Titan Probe and Radar Mapper’.

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Notes

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(2007). Cassini-Huygens. In: Cassini at Saturn. Springer Praxis Books. Praxis. https://doi.org/10.1007/978-0-387-73978-6_5

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