Difference between revisions of "Oppenheimer Station"

From Bravo Fleet
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| name = Oppenheimer Station
| name = Oppenheimer Station
| image =  
| image =  
[[File:Oppenhimer Research Outpost.jpg|300px|none|center|Oppenhimer Research Outpost]]
[[File:Oppenheimer station.jpg|500px|none|center|Oppenhiemer Research Outpost]]
| registry =  
| registry =  
| class = [[Regula Class]]
| class = [[Regula Class]]

Revision as of 16:25, 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.

<<STAR MAP TO BE ADDED HERE>>

Orbital Characteristics