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Descripción
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| Search for habitability in moons of Outer planets, requires presence of water, energy, and proper chemistry. Dissipation from tidal forces is a major energy source in evolution of Icy moon systems. Saturn moons Enceladus and Dione are in a 1:2 Laplace resonance. Enceladus ejects plumes of water vapor and ice particles, Dione exhibits linear virgae, hundred kilometres long, latitudinal color lines. A minor tether mission would explore this system. Following Saturn capture, repeated, free Lorentz drag at periapsis brings apoapsis to elliptical orbit at 1:1 resonance with Dione. After multiple flybys, repeated operation reaches 1:2 resonance with Enceladus, for flybys. | |
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Internacional
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Si |
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Nombre congreso
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8th European Conference for Aeronautics and Space Sciences (EUCASS 2019) |
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Tipo de participación
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960 |
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Lugar del congreso
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ETSI Aeronáutica y del Espacio, Universidad Politécnica de Madrid, Madrid, Spain |
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Revisores
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Si |
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ISBN o ISSN
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DOI
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10.13009/EUCASS2019-81 |
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Fecha inicio congreso
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01/07/2019 |
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Fecha fin congreso
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04/07/2019 |
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Desde la página
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1 |
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Hasta la página
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7 |
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Título de las actas
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8th European Conference for Aeronautics and Space Sciences (EUCASS 2019) |