in the rings of Saturn. Career Voyager In the fall of 1983, Porco joined the faculty of the Department of Planetary Sciences at the University of Arizona; the same year she was made a member of the Voyager Imaging Team. In the latter capacity, she was an active participant in the Voyager 2 encounters with Uranus in 1986 and Neptune in 1989, leading the Rings Working Group within the Voyager Imaging Team during the Neptune encounter. Porco was the first person to describe the behavior of the eccentric ringlets and the "spokes" discovered by Voyager within the rings of Saturn; to elucidate the mechanism by which the outer Uranian rings were being shepherded by the Voyager-discovered moons Cordelia and Ophelia; and to provide an explanation for the shepherding of the rings arcs of Neptune by the moon Galatea, also discovered by Voyager. She was a co-originator of the idea to take a 'portrait of the planets' with the Voyager 1 spacecraft, and participated in the planning, design, and execution of those images in 1990, including the famous Pale Blue Dot image of Earth. Cassini–Huygens In November 1990, Porco was selected as the leader of the Imaging Team for the Cassini-Huygens mission, an international mission that successfully placed a spacecraft in orbit around Saturn and deployed the atmospheric Huygens probe to Saturn's largest satellite, Titan. She is also the Director of the Cassini Imaging Central Laboratory for Operations (CICLOPS), which was the center of uplink and downlink operations for the Cassini imaging science experiment and the place where Cassini images are processed for release to the public. CICLOPS is part of the Space Science Institute in Boulder, Colorado. In the course of the ongoing mission, Porco and her team have discovered seven moons of Saturn: Methone and Pallene, Polydeuces, Daphnis, Anthe, Aegaeon, and a small moonlet in the outer B ring. They also found several new rings, such as rings coincident with the orbits of Atlas, Janus and Epimetheus (the Saturnian 'co-orbitals') and Pallene; a diffuse ring between Atlas and the F ring; and new rings within several of the gaps in Saturn's rings. In 2013, Cassini data confirmed a 1993 prediction by Porco and Mark Marley that acoustic oscillations within the body of Saturn are responsible for creating particular features in the rings of Saturn. This confirmation, the first to demonstrate that planetary rings can act like a seismograph in