- Cassini RADAR
The Radio Detection and Ranging Instrument (RADAR) onboard the Cassini orbiter will be used to measure 3 modes of data: radiometry, altimetry and imaging on Saturn's moon, Titan.
- Cosmic Dust Analyzer CDA
- ESA Site
ESA's Cassini-Huygens website features news, status reports on the mission, images, videos, live streaming and much more! The Huygens mission is the ESA-provided element of the international Cassini-Huygens mission to Saturn and Titan jointly developed by NASA and ESA. The primary scope of the mission is to descend through the atmosphere of Titan, Saturn's largest moon, making m
cassini exploration huygens mission saturn space titan
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- Imaging Subsystem CICLOPS
Public web site for CICLOPS, the Cassini Imaging Central Laboratory for Operations
- Infrared Spectrometer CIRS
- Ion & Mass Spectrometer INMS
The Ion and Neutral Mass Spectrometer (INMS) onboard the Cassini orbiter is designed to measure the positive ion and neutral species structure and composition in Saturn's magnetosphere and upper atmosphere of Titan.
- JPL Site
The Cassini-Huygens Mission to the Saturnian system is a multinational cooperation between three space agencies and 17 nations. Starting in 2004, the spacecraft will explore Saturn, its mysterious rings and its many moons. The Cassini spacecraft will orbit the ringed planet for four years. The Huygens probe will dive into the atmosphere of Titan, Saturn's biggest moon.
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- Magnetometer MAG
- Magnetospheric Imaging MIMI
- Plasma Spectrometer CAPS
- Radio & Plasma Wave RPWS
- Radio Science RSS
The Radio Science Subsystem (RSS) onboard the Cassini orbiter is designed to study the compositions, pressures and atmospheric temperatures around Saturn, its rings, and around gravitational waves.
- Ultraviolet Spectrograph UVIS
The Ultraviolet Imaging Spectrograph (UVIS) onboard the orbiter Cassini is a valuable instrument, used to measure the composition, distribution of Saturn's atmospheres both spectrally and spatially.
- Visual/Infrared Spectrom. VIMS
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