Station
Similar stations in Paresa
Surface Port - 147 Ls
Peraesii Empire Consulate
Khrenov Depot
Surface Port - 147 Ls
Peraesii Empire Consulate
Stott Horizons
Surface Port - 147 Ls
Peraesii Empire Consulate
Dyson City
Starport (Coriolis) - 260 Ls
Nova Paresa
Koishikawa Port
Starport (Orbis) - 354 Ls
Peraesii Empire Consulate
Kahn Orbital
Starport (Orbis) - 355 Ls
Nova Paresa
Knight Base
Surface Port - 473 Ls
Peraesii Empire Consulate
Alexandrov Vista
Surface Port - 1,929 Ls
Peraesii Empire Consulate
Baker Depot
Surface Port - 1,929 Ls
Peraesii Empire Consulate
Galpedia
Carolyn Porco
Carolyn C. Porco (born March 6, 1953) is an American planetary scientist known for her work in the exploration of the outer solar system, beginning with her imaging work on the Voyager missions to Jupiter, Saturn, Uranus, and Neptune in the 1980s. She leads the imaging science team on the Cassini mission currently in orbit around Saturn. She is also an imaging scientist on the New Horizons mission launched to Pluto on January 19, 2006. She is an expert on planetary rings and the Saturnian moon, Enceladus.
She has co-authored more than 110 scientific papers on subjects ranging from the spectroscopy of Uranus and Neptune, the interstellar medium, the photometry of planetary rings, satellite/ring interactions, computer simulations of planetary rings, the thermal balance of Triton’s polar caps, heat flow in the interior of Jupiter, and a suite of results on the atmosphere, satellites, and rings of Saturn from the Cassini imaging experiment. 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.
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