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The Complete Book of Spaceflight: From Apollo 1 to Zero Gravity

The Complete Book of Spaceflight: From Apollo 1 to Zero Gravity

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Cassini orbiter<br />

Experiments aboard the orbiter include: the Imaging Science<br />

Subsystem, the Cassini Radar, the Radio Science<br />

Subsystem, the Ion and Neutral Mass Spectrometer, the<br />

Visible and Infrared Mapping Spectrometer, the Composite<br />

Infrared Spectrometer, the Cosmic Dust Analyzer,<br />

the Radio and Plasma Wave Spectrometer, the Cassini<br />

Plasma Spectrometer, the Ultraviolet Imaging Spectrograph,<br />

the Magne<strong>to</strong>spheric Imaging Instrument, and the<br />

Dual Technique Magne<strong>to</strong>meter. Cassini is about the size<br />

<strong>of</strong> a 30-passenger school bus and one <strong>of</strong> the largest interplanetary<br />

spacecraft ever launched.<br />

Huygens probe<br />

<strong>The</strong> ESA component <strong>of</strong> the Cassini mission, named for<br />

the Dutch scientist Christaan Huygens (1629–1695), who<br />

discovered Titan. It will be released in December 2004<br />

and enter Titan’s atmosphere on January 14, 2005. Initially,<br />

the 2.7-m diameter probe will use its heat shield <strong>to</strong><br />

Cassini 69<br />

Cassini Cassini being prepared for launch.<br />

NASA<br />

Cassini (Huygens probe) An artist’s rendering <strong>of</strong> the Huygens<br />

probe descending <strong>to</strong> the surface <strong>of</strong> Titan. European Space Agency

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