Wregoe YI-W b32-0
X: -54.71875 / Y: 621.875 / Z: -351.65625
Updated
25d 9h
25d 9h
System Governance
Minor faction ---
Allegiance None
Government None
Security Anarchy
Population 0
Economy & Assets
Primary None
Secondary None
Stellar Bodies 4
Stations 0
Fuel scoop
Available
Wregoe YI-W b32-0 A
M (Red dwarf) Star
Fuel scoop
Subclass2
LuminosityVa
Distance0.00ls
Stellar Mass0.40
Radius428,617,152.00
Absolute Magnitude8.38
Rotation Period169,429.77
Surface Temperature3254
Age4580
Axial Tilt0.00
Semi-Major Axis948,213,112.35
Eccentricity0.01
Orbital Inclination-5.60
Periapsis205.15
Orbital Period75,258.65
Ascending Node-38.15
Mean Anomaly230.94
Wregoe YI-W b32-0 B
M (Red dwarf) Star
Fuel scoop
Subclass7
LuminosityVa
Distance7.86ls
Stellar Mass0.27
Radius335,948,896.00
Absolute Magnitude10.07
Rotation Period206,520.24
Surface Temperature2489
Age4580
Axial Tilt0.00
Semi-Major Axis1,395,228,207.11
Eccentricity0.01
Orbital Inclination-5.60
Periapsis25.15
Orbital Period75,258.65
Ascending Node-38.15
Mean Anomaly230.95
Wregoe YI-W b32-0 C
L (Brown dwarf) Star
Subclass3
LuminosityV
Distance1,565.79ls
Stellar Mass0.14
Radius206,922,272.00
Absolute Magnitude12.67
Rotation Period107,298.56
Surface Temperature1741
Age4580
Axial Tilt0.00
Semi-Major Axis482,530,295,848.85
Eccentricity0.32
Orbital Inclination-1.34
Periapsis253.31
Orbital Period269,918,590.78
Ascending Node145.45
Mean Anomaly36.96
Wregoe YI-W b32-0 D
M (Red dwarf) Star
Fuel scoop
Subclass2
LuminosityVa
Distance228,333.42ls
Stellar Mass0.40
Radius389,159,904.00
Absolute Magnitude8.59
Rotation Period224,274.75
Surface Temperature3250
Age4580
Axial Tilt0.00
Semi-Major Axis35,798,418,521,881.10
Eccentricity0.29
Orbital Inclination5.70
Periapsis351.70
Orbital Period191,592,669,487.00
Ascending Node103.59
Mean Anomaly161.81
| System | Minor faction | Population | Security | Distance | Scoopable |
|---|---|---|---|---|---|
| Wregoe QC-X c16-0📋 | 0 | Anarchy | 19.79 | Yes | |
| Wregoe QC-X c16-1📋 | 0 | Anarchy | 21.22 | No | |
| Wredguia LG-W b32-0📋 | 0 | Anarchy | 35.60 | No |