Station
Similar stations in HIP 4668
Outpost (Civilian) - 55 Ls
Confederacy of British Commanders
Mil Terminal
Outpost (Civilian) - 78 Ls
Confederacy of British Commanders
Seamans Orbital
Outpost (Civilian) - 167 Ls
Confederacy of British Commanders
Lee Dock
Outpost (Mining) - 376 Ls
Nisgan Jet Vision Services
Koishikawa Hub
Outpost (Industrial) - 377 Ls
Nisgan Jet Vision Services
Curtiss Orbital
Starport (Orbis) - 2,370 Ls
Confederacy of British Commanders
McKie Hub
Starport (Coriolis) - 2,513 Ls
HIP 4668 Patrons of Law
Weaver Orbital
Starport (Coriolis) - 2,513 Ls
HIP 4668 Patrons of Law
Graham Port
Starport (Coriolis) - 2,555 Ls
Nisgan Jet Vision Services
Bouvard Settlement
Surface Port - 2,616 Ls
HIP 4668 Patrons of Law
Moore Vista
Surface Station - 2,798 Ls
HIP 4668 Patrons of Law
Spurzem Palace
Surface Station - 3,074 Ls
Nisgan Jet Vision Services
Galpedia
Eugene Parker
Eugene N. Parker (born June 10, 1927) is an American solar astrophysicist who received his B.S. degree in physics from Michigan State University in 1948 and Ph.D. from Caltech in 1951. In the mid-1950s Parker developed the theory on the supersonic solar wind and predicted the Parker spiral shape of the solar magnetic field in the outer solar system. In 1987, Parker proposed that the solar corona might be heated by myriad tiny "nanoflares", miniature brightenings resembling solar flares that would occur all over the surface of the Sun.
Parker was elected to the National Academy of Sciences in 1967. As of early 2005, he was still engaged in active research at the University of Chicago. His daughter and son-in-law are both faculty members at Michigan State University.
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