Difference between revisions of "Oppenheimer Station"
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Both stars have planets but only '''γ CrB - B''' has bodies that have low orbital eccentricity. | Both stars have planets but only '''γ CrB - B''' has bodies that have low orbital eccentricity. | ||
[[File:Oppenheimer map.jpg|thumb|System Location ]] | |||
==== Orbital Characteristics ==== | ==== Orbital Characteristics ==== | ||
Revision as of 16:40, 9 May 2023
Oppenheimer Station (also known as Oppenheimer Research Outpost) is a Regula Class station located in the Gamma Coronae Borealis system (abbreviated γ CrB).
The facility is fairly unusual in that it is anchored at the L4 Lagrange point with its two parent bodies being the γ CrB - B star and the γ CrB - B6 planet . Over millennia the L4 Lagrange point has accumulated a large amount of stellar debris and dust resulting in the formation of a large Ionised dust cloud that resembles a small micro-nebula
Location
Oppenhiemer station is located in the Gamma Coronae Borealis system which is approximately 18 Light years Coreward from Farpoint Station. γ CrB is a binary star system containing a primary star ( γ CrB - A) of spectral classification B9 V and a secondary star ( γ CrB - B) of spectral classification A3 V.
Both stars have planets but only γ CrB - B has bodies that have low orbital eccentricity.
