Difference between revisions of "Oppenheimer Station"
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== Location == | == Location == | ||
Oppenhiemer station is located in the Gamma Coronae Borealis system which is approximately 18 Light years Coreward from [[Farpoint Station|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.<gallery widths=" | Oppenhiemer station is located in the Gamma Coronae Borealis system which is approximately 18 Light years Coreward from [[Farpoint Station|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.<gallery widths="500" heights="324"> | ||
File:Oppenheimer map.jpg|System Location | File:Oppenheimer map.jpg|System Location | ||
</gallery>Both stars have planets but only '''γ CrB - B''' has bodies that have low orbital eccentricity. | </gallery>Both stars have planets but only '''γ CrB - B''' has bodies that have low orbital eccentricity. | ||
==== Orbital Characteristics ==== | ==== Orbital Characteristics ==== |
Revision as of 16:43, 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