Cassini imaging scientists used views like this one to help them identify the source locations for individual jets spurting ice particles, water vapour and trace organic compounds from the surface of Saturn's moon Enceladus. Their study -- published in the Oct. 11, 2007, issue of the journal Nature -- identifies eight source locations, all on the prominent tiger stripe fractures, or sulci, in the moon's south polar region. Some of the sources occur in regions not yet observed by Cassini's composite infrared spectrometer, and the researchers predict that future Cassini observations of those locations will find elevated temperatures.
This image product was then specially processed to enhance the individual jets that compose the plume. Some artefacts due to the processing are present in the image. The final product was coloured as blue for dramatic effect. The images were acquired with the Cassini spacecraft narrow-angle camera on Nov. 27, 2005 at a distance of approximately 148,000 kilometres from Enceladus and at a sun-Enceladus-spacecraft, or phase, angle of 161 degrees.
This map of the south polar region of Saturn's moon Enceladus shows the correlation between jet sources identified in Cassini imaging data and hot spots on the surface located by the composite infrared spectrometer instrument. To identify jet source locations on the surface, imaging scientists carefully measured the locations and orientations of individual jets observed along the moon's limb in Cassini images taken from multiple viewing angles. For each jet measurement, the researchers then computed a curve, or ground track, on the surface of Enceladus along which that jet might lie. The ground tracks from all of the measurements made in the various images produced many intersections on this map. By considering the jet directions at every possible intersection, the researchers isolated eight clusters of ground track intersections as jet sources.
The eight identified jet source locations are labelled with yellow roman numerals. Composite infrared spectrometer hot spots are red boxes labelled with green capital letters. The line-of-sight intersections indicating the measurements of each source in individual images are shown as coloured diamonds. White circles indicate the uncertainty in the locations of those sets of intersections. The map is a polar stereographic projection of Cassini imaging data. The four tiger stripe fractures, or sulci, are labelled here. The south pole is dead centre on the map. Key longitudes are also labelled around the perimeter of the map.
Tiny grains of ice or particles of space dust could significantly damage the Cassini spacecraft when it passes close by Saturns moon Enceladus next March, scientists said Thursday. Images from Cassini beamed back to Earth in 2005 showed multiple jets emanating from the moons south polar region that scientists suspect arise from warm fractures, known as tiger stripes.
A new model of Saturn's icy moon Enceladus may quell hopes of finding life there. Developed by researchers at the University of Illinois, the model explains the most salient observations on Enceladus without requiring the presence of liquid water.
This nearly equatorial mage of Enceladus was taken in polarised green light with the Cassini spacecraft narrow-angle camera on June 28, 2007, when it was approximately 293,000 kilometres away.
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The Cassini spacecraft will perform its closest flyby ever of Saturn's ice-spewing moon Enceladus early next year, moving directly into its polar geyser for a deep-space shower. Cassini's third flyby of Enceladus, set for March 2008, will swing it within 30 kilometres of the Saturnian moon almost six times closer than the spacecraft's closest pass to it in 2005.
The movie was created from 40 original images taken over the course of about 20 minutes as the spacecrafts narrow angle camera remained pointed toward Enceladus. Additional frames were inserted between the 40 Cassini images in order to smooth the appearance of the moons movement. As Enceladus approaches Rhea, the shadow of Saturn can be seen, projected onto the unlit side of its rings.
The images were taken in visible light with the Cassini spacecraft narrow-angle camera on March 2, 2006 at a distance of approximately 2.8 million kilometres from Rhea and 2 million kilometres from Enceladus. Image scale is 17 kilometres per pixel on Rhea and 12 kilometres per pixel on Enceladus.
The Cassini spacecraft will perform its closest flyby ever of Saturn's ice-spewing moon Enceladus early next year, moving directly into its icy polar geyser for a deep-space shower. Cassini's third flyby of Enceladus, set for March 2008, will swing it within 30 kilometres of the saturnian moon - almost six times closer than the spacecraft's closest pass to it in 2005. The trajectory will move Cassini directly into the icy geyser at the moon's southern pole.
"Cassini was never designed to fly this close, but we've just got to get in that plume and look at that material and see what it is and where it's coming from" - James Green, director of NASA's Planetary Division in Washington, D.C.
This image shows Enceladus moving in front of Tethys and was taken by the Cassini spaceprobe on July 24, 2007, when Enceladus was approximately 1,875,769 kilometres away, and Tethys was approximately 2,040,982 kilometres away.
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The image was taken using the CL1 and CL2 filters.
This image also shows Enceladus and Tethys and was taken by the Cassini spaceprobe on July 25, 2007.
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The image was taken using the P120 and GRN filters.