THE SATURN SYSTEM

This montage of images of the Saturnian System was prepared from an assemblage of images taken by the Voyager 1 spacecraft during its Saturn encounter in November 1980. This artist's arrangement shows Dione in the forefront, Saturn rising behind, Tethys and Mimas fading in the distance to the right, Enceladus and Rhea off Saturn's rings to the left, and Titan in its distant orbit at the top. With a diameter of 5150 km (3200 mi), Titan is by far the largest of the Saturn satellites and is the only moon in the Solar System with an Earth-sized atmosphere. Heavily cratered Rhea, whose diameter is 1530 km (950 mi), is Saturn's second largest satellite. Tethys and Dione are about 1100 km (680 mi) in diameter. 500-km (310-mi) Enceladus may be the source of the tiny ice particles which form Saturn's tenuous E ring. 392-km (244-mi) Mimas, with the enormous crater Herschel on one side, has an appearance reminiscent of the Death Star in the movie "Star Wars." (P-23209)