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="500" heights="324">
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" mode="nolines">
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 16:44, 9 May 2023

[[Category:Regula Class-class]]


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.

Orbital Characteristics