Difference between revisions of "Oppenheimer Station"
| Line 5: | Line 5: | ||
| registry = | | registry = | ||
| class = [[Regula Class]] | | class = [[Regula Class]] | ||
| affiliation = [[United Federation of Planets]] | | affiliation = Independant (Formerly [[United Federation of Planets]]) | ||
| status = Active | | status = Active | ||
| commissioned = 2368 | | commissioned = 2368 | ||
Revision as of 03:38, 9 May 2023
 | |
| Oppenheimer Station | |
| Information | |
| Class | |
| Affiliation |
Independant (Formerly United Federation of Planets) |
| Status | Active |
| Commissioned | 2368 |
| Location | |
| System | Gamma Coronae Borealis |
| Sector | Deneb Sector |
| Quadrant | Alpha Quadrant |
| Assignment | |
| Role |
Research Outpost |
| Template:Starbase | |
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>>