This still is from a short computer-animated film that highlights Cassini's accomplishments at Saturn and reveals the science-packed final orbits.
This website is the PDS home page for the Cassini mission to Saturn. It has information to help understand the spacecraft and mission,
the instrument payload, details about how to find, calibrate, and analyze data from each instrument, and resources to help
find more information about the core science areas that have been studied in the Saturn system. For detailed information regarding the Huygens probe, visit the European Space Agency's website.
OVERVIEW
MISSION SCIENCE AREAS
The pages below summarize research on the key science targets in the Saturn system and how each target was studied by the Cassini spacecraft.
Science Targets
science includes Saturn's formation and evolution, interior fundamentals, atmospheric properties, global circulation and dynamics, auroral observations, ionosphere and magnetic fields.
science includes the configuration and process responsible for ring structure, composition, relationships with satellites, and interactions with Saturn's magnetosphere, ionosphere and atmosphere.
science includes the configuration of Saturn's magnetic field, distribution of charged particles in the magnetosphere, Saturn's aurorae, and Titan's interaction with the magnetospheric plasma.
science includes interior studies, surface investigations, Huygens Lander data, atmosphere and Magnetospheric interactions.
science includes the study of Enceladus, other icy satellites such as Dione, small moons such as Phoebe, and the ring-moon relationships.
science includes atmosphere, rings and moons data collected during the Cassini flyby of Jupiter.
INSTRUMENTS
The pages below summarize the instrument capabilities and science applications, provide links to extensive documentation, as well as links to data search and data analysis tools.
Optical Remote Sensing instruments
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Infrared studies of temperature and composition of surfaces, atmospheres and rings within the Saturn system
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Multispectral imaging of Saturn, Titan, rings and icy satellites to observe their properties
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Ultraviolet spectra and low-resolution imaging of atmospheres and rings for structure, chemistry and composition
Visible and infrared spectral mapping to study composition and structure of surfaces, atmospheres and rings
Radio Instruments
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RADAR imaging, altimetry, and passive radiometry of Titan's surface
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Study of atmospheric and ring structure, gravity fields and gravitational waves
Fields and Particles instruments
Study of plasma within and near Saturn's magnetic field
Study of ice and dust grains in the Saturn system
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Study of compositions of neutral and charged particles within the magnetosphere
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Study of Saturn's magnetic field and interactions with the solar wind
Global magnetospheric imaging and measurements of Saturn's magnetosphere and solar wind interactions
Measurement of electric and magnetic fields, and electron density and temperature in the interplanetary medium and within Saturn's magnetosphere