Abstract
The Cassini visual and infrared mapping spectrometer (VIMS) investigation
is a multidisciplinary study of the Saturnian system. Visual and
near-infrared imaging spectroscopy and high-speed spectrophotometry
are the observational techniques. The scope of the investigation
includes the rings, the surfaces of the icy satellites and Titan,
and the atmospheres of Saturn and Titan. In this paper, we will elucidate
the major scientific and measurement goals of the investigation,
the major characteristics of the Cassini VIMS instrument, the instrument
calibration, and operation, and the results of the recent Cassini
flybys of Venus and the Earth-Moon system.
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