Station
Similar stations in HIP 107010
Surface Port - 144 Ls
HIP 107010 Citizens of Tradition
Baynes Terminal
Outpost (Civilian) - 144 Ls
Celestial Light Brigade
Cook Works
Surface Port - 144 Ls
HIP 107010 Citizens of Tradition
Herbert Reach
Surface Port - 144 Ls
HIP 107010 Limited
Mayer Enterprise
Surface Port - 144 Ls
HIP 107010 Citizens of Tradition
Lalande Dock
Outpost (Civilian) - 246 Ls
Celestial Light Brigade
Flammarion Dock
Outpost (Civilian) - 445 Ls
HIP 107010 Citizens of Tradition
Gorbatko Horizons
Surface Port - 445 Ls
Celestial Light Brigade
Farghani Ring
Starport (Orbis) - 820 Ls
Celestial Light Brigade
Watson Port
Outpost (Civilian) - 2,714 Ls
HIP 107010 Limited
Rustah Bastion
Surface Port - 74,941 Ls
HIP 107010 Limited
Petlyakov Point
Surface Port - 75,014 Ls
Celestial Light Brigade
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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