Zunia AD-R c18-168
X: 9012.0625 / Y: 90.5 / Z: 24083.53125
Updated
51d 16h
51d 16h
System Governance
Minor faction ---
Allegiance None
Government None
Security Anarchy
Population 0
Economy & Assets
Primary None
Secondary None
Stellar Bodies 2
Stations 0
Fuel scoop
Available
Zunia AD-R c18-168 A
K (Yellow-Orange) Star
Fuel scoop
Subclass7
LuminosityVa
Distance0.00ls
Stellar Mass0.59
Radius518,228,960.00
Absolute Magnitude6.99
Rotation Period281,008.14
Surface Temperature4070
Age2864
Axial Tilt0.00
Semi-Major Axis782,186,722,755.43
Eccentricity0.01
Orbital Inclination-91.98
Periapsis105.88
Orbital Period3,830,829,799.18
Ascending Node-36.92
Mean Anomaly195.62
Zunia AD-R c18-168 B
M (Red dwarf) Star
Fuel scoop
Subclass9
LuminosityVI
Distance11,391.35ls
Stellar Mass0.18
Radius223,838,560.00
Absolute Magnitude11.73
Rotation Period132,416.97
Surface Temperature2081
Age2864
Axial Tilt0.00
Semi-Major Axis2,584,617,137,908.94
Eccentricity0.01
Orbital Inclination-91.98
Periapsis285.88
Orbital Period3,830,829,799.18
Ascending Node-36.92
Mean Anomaly195.62
| System | Minor faction | Population | Security | Distance | Scoopable |
|---|---|---|---|---|---|
| Zunia EN-N a76-0π | 0 | Anarchy | 7.60 | No | |
| Zunia DR-G b38-32π | 0 | Anarchy | 7.70 | Yes | |
| Zunia NO-I d9-702π | 0 | Anarchy | 9.53 | Yes | |
| Zunia YH-R c18-97π | 0 | Anarchy | 12.18 | Yes | |
| Zunia DR-G b38-44π | 0 | Anarchy | 14.01 | Yes | |
| Zunia ER-G b38-14π | 0 | Anarchy | 16.19 | Yes | |
| Zunia FJ-P c19-299π | 0 | Anarchy | 16.83 | Yes | |
| Zunia CO-P c19-208π | 0 | Anarchy | 17.63 | Yes | |
| Zunia FJ-P c19-157π | 0 | Anarchy | 20.06 | Yes | |
| Zunia PU-J a78-0π | 0 | Anarchy | 20.27 | No | |
| Zunia HX-E b39-61π | 0 | Anarchy | 20.44 | Yes | |
| Zunia AH-P a75-1π | 0 | Anarchy | 21.27 | No | |
| Zunia FJ-P c19-146π | 0 | Anarchy | 22.92 | Yes | |
| Zunia NO-I d9-121π | 0 | Anarchy | 24.46 | Yes | |
| Zunia NO-I d9-681π | 0 | Anarchy | 27.05 | Yes | |
| Zunia AD-R c18-28π | 0 | Anarchy | 30.17 | Yes | |
| Zunia XV-Q a74-0π | 0 | Anarchy | 32.61 | No |