This picture is a mosaic of six images—two each via red, green and blue spectral filters—combined to create this natural color view. The images were obtained with the Cassini spacecraft wide-angle camera on 6 May, 2012. The view looks toward the northern, sunlit side of the rings from just above the ring plane.
The giant moon Titan is silhouetted in front of Saturn as the planet is changing seasons. Titan, Saturn’s largest moon, measures 35,150 km across and is larger than the planet Mercury. It could have been a planet if it were on its own.
Saturn’s southern hemisphere, in its approach to winter, is taking on a bluish hue. This change seems to be caused by a reduced intensity of ultraviolet light. UV produces haze in Saturn’s atmosphere, and the increasing intensity of ultraviolet light in the hemisphere approaching summer causes the increase in haze. The presence of the ring shadow in the winter hemisphere enhances this effect. The reduction of smog and the consequent clearing of the atmosphere makes for a bluish hue. The presence of methane, which generally absorbs in the red part of the spectrum, in a now clearer atmosphere also enhances the blue. A different mechanism, the increased opportunity for direct scattering of sunlight by the molecules in the air, makes the sky blue, as on Earth.
Image Credit: NASA