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Enceladus and the Icy Moons of Saturn
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With active geysers coating its surface with dazzlingly bright ice crystals, Saturn’s large moon Enceladus is one of the most enigmatic worlds in our solar system. Underlying this activity are numerous further discoveries by the Cassini spacecraft, tantalizing us with evidence that Enceladus harbors a subsurface ocean of liquid water. Enceladus is thus newly realized as a forefront candidate among potentially habitable ocean worlds in our own solar system, although it is only one of a family of icy moons orbiting the giant ringed planet, each with its own story.
As a new volume in the Space Science Series, Enceladus and the Icy Moons of Saturn brings together nearly eighty of the world’s top experts writing more than twenty chapters to set the foundation for what we currently understand, while building the framework for the highest-priority questions to be addressed through ongoing spacecraft exploration. Topics include the physics and processes driving the geologic and geophysical phenomenon of icy worlds, including, but not limited to, ring-moon interactions, interior melting due to tidal heating, ejection and reaccretion of vapor and particulates, ice tectonics, and cryovolcanism.
By contextualizing each topic within the profusion of puzzles beckoning from among Saturn’s many dozen moons, Enceladus and the Icy Moons of Saturn synthesizes planetary processes on a broad scale to inform and propel both seasoned researchers and students toward achieving new advances in the coming decade and beyond.
As a new volume in the Space Science Series, Enceladus and the Icy Moons of Saturn brings together nearly eighty of the world’s top experts writing more than twenty chapters to set the foundation for what we currently understand, while building the framework for the highest-priority questions to be addressed through ongoing spacecraft exploration. Topics include the physics and processes driving the geologic and geophysical phenomenon of icy worlds, including, but not limited to, ring-moon interactions, interior melting due to tidal heating, ejection and reaccretion of vapor and particulates, ice tectonics, and cryovolcanism.
By contextualizing each topic within the profusion of puzzles beckoning from among Saturn’s many dozen moons, Enceladus and the Icy Moons of Saturn synthesizes planetary processes on a broad scale to inform and propel both seasoned researchers and students toward achieving new advances in the coming decade and beyond.
作者簡介
Paul M. Schenk is a staff scientist at the Lunar and Planetary Institute in Houston, Texas.
Roger N. Clark is a senior scientist at the Planetary Science Institute in Tucson, Arizona.
Carly J. A. Howett is a section manager for the Outer Solar System Section in the Division of Space Science and Engineering at the Southwest Research Institute in Boulder, Colorado.
Anne J. Verbiscer is a research professor in the Department of Astronomy at University of Virginia in Charlottesville.
J. Hunter Waite is a program director for the Division of Space Science and Engineering at the Southwest Research Institute in San Antonio, Texas.
Roger N. Clark is a senior scientist at the Planetary Science Institute in Tucson, Arizona.
Carly J. A. Howett is a section manager for the Outer Solar System Section in the Division of Space Science and Engineering at the Southwest Research Institute in Boulder, Colorado.
Anne J. Verbiscer is a research professor in the Department of Astronomy at University of Virginia in Charlottesville.
J. Hunter Waite is a program director for the Division of Space Science and Engineering at the Southwest Research Institute in San Antonio, Texas.
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