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Flyby of Rhea Cassini swoops down to within about 100 kilometers (More) Cassini swoops down to within about 100 kilometers of Rhea to 'sniff' the moon. Particle and fields instruments will try to determine what is coming off Rhea. The last targeted flyby of Rhea happened in November 2005. Approaching Rhea, RADAR performs a raster scan of the moon's surface to obtain simultaneous scatterometry and radiometry measurements to understand the texture and composition of the surface. The Cassini Plasma Spectrometer (CAPS) takes over prime pointing 45 minutes before closest approach to observe the interaction before Rhea and Saturns magnetosphere. After closest approach, the Visible and Infrared Mapping Spectrometer (VIMS) and the Composite Infrared Spectrometer (CIRS) will image Rhea at visible and infrared wavelengths to better understand its geologic history and composition, and CIRS will continue to observe while Rhea goes into eclipse. (Less)
Rhea's Blue Streaks The Cassini orbiter has revealed many surprises (More) The Cassini orbiter has revealed many surprises within the Saturn system, including the possible presence of a ring of debris surrounding the ancient heavily cratered surface of Rhea, Saturn's second largest moon. Until now, no direct visual evidence of Rhea's suspected ring has been detected. This perspective view shows one of a series of relatively blue patches that form a very narrow band only 10 kilometers wide that straddles Rhea's equator. This view was created using stereo topography generated by Dr. Paul Schenk (www.lpi.usra.edu of the Lunar and Planetary Institute in Houston Texas from Cassini imaging data returned in 2008. The bluish material is believed to be fresh ice reexposed when material from Rhea's ring struck the surface along the equator, and is a target of investigation for the March 2 Cassini flyby of Rhea. The largest craters shown here are about 20 to 30 kilometers wide and 3 to 5 kilometers deep. The colors have been enhanced to highlight the color differences between these patches and the more typical cratered terrains of Rhea. credit: NASA / JPL / Space Science Institute / Universities Space Research Association / Lunar & Planetary Institute source: photojournal.jpl.nasa.gov (Less)
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