View of Saturn’s rings during equinox

via CICLOPS

[…] Seen from our planet, the view of Saturn’s rings during equinox is extremely foreshortened and limited. But in orbit around Saturn, Cassini had no such problems. From 20 degrees above the ringplane, Cassini’s wide angle camera shot 75 exposures in succession for this mosaic showing Saturn, its rings, and a few of its moons a day and a half after exact Saturn equinox, when the sun’s disk was exactly overhead at the planet’s equator.

The novel illumination geometry that accompanies equinox lowers the sun’s angle to the ringplane, significantly darkens the rings, and causes out-of-plane structures to look anomalously bright and to cast shadows across the rings. These scenes are possible only during the few months before and after Saturn’s equinox which occurs only once in about 15 Earth years. […]

The images comprising the mosaic, taken over about eight hours, were extensively processed before being joined together. First, each was reprojected into the same viewing geometry and then digitally processed to make the image “joints” seamless and to remove lens flares, radially extended bright artifacts resulting from light being scattered within the camera optics. […]

The images were taken on Aug. 12, 2009, beginning about 1.25 days after exact equinox, using the red, green and blue spectral filters of the wide angle camera and were combined to create this natural color view. The images were obtained at a distance of approximately 847,000 kilometers (526,000 miles) from Saturn and at a Sun-Saturn-spacecraft, or phase, angle of 74 degrees. Image scale is 50 kilometers (31 miles) per pixel. […]

Coming to light

via CICLOPS

Again, a fantastic view of Saturn.

As seasons change on Saturn, and sunlight creeps farther north, the region surrounding the north pole is steadily coming to light.

This scene reveals many features in Saturn’s dynamic and beautiful atmosphere, including a detail largely obscured from the imaging cameras until now. On the terminator at center right is part of the polar hexagon, which was previously observed by Cassini’s Visible and Infrared Mapping Spectrometer (VIMS) and Composite Infrared Spectrometer (CIRS). These instruments used heat radiated from Saturn to observe the polar hexagon (rather than reflected sunlight, as is the case in this view). The hexagon was first imaged by the Voyager spacecraft more than 25 years ago.

The view looks toward the unilluminated side of the rings from about 38 degrees above the ringplane and is centered on a region 63 degrees north of the Saturnian equator.

The image has been brightened to show details at high northern latitudes, where solar illumination is presently weak.