HIP 107462
X: -584.90625 / Y: -229.71875 / Z: 111.96875
Updated
13d 18h
13d 18h
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
HIP 107462 A
B (Blue-White) Star
Fuel scoop
Subclass9
LuminosityIV
Distance0.00ls
Stellar Mass2.87
Radius1,428,653,056.00
Absolute Magnitude0.38
Rotation Period51,759.11
Surface Temperature11822
Age802
Axial Tilt0.00
Semi-Major Axis213,000,959,157.94
Eccentricity0.05
Orbital Inclination46.33
Periapsis266.26
Orbital Period120,315,843.82
Ascending Node102.58
Mean Anomaly174.56
HIP 107462 B
F (White) Star
Fuel scoop
Subclass2
LuminosityVb
Distance2,106.46ls
Stellar Mass1.58
Radius855,833,408.00
Absolute Magnitude3.45
Rotation Period106,466.03
Surface Temperature7161
Age802
Axial Tilt0.00
Semi-Major Axis387,514,227,628.71
Eccentricity0.05
Orbital Inclination46.33
Periapsis86.26
Orbital Period120,315,843.82
Ascending Node102.58
Mean Anomaly174.56
| System | Minor faction | Population | Security | Distance | Scoopable |
|---|---|---|---|---|---|
| Synuefai CA-G c27-10π | 0 | Anarchy | 10.77 | Yes | |
| Synuefai NU-D d13-64π | 0 | Anarchy | 15.14 | Yes | |
| Synuefai NU-D d13-56π | 0 | Anarchy | 18.83 | Yes | |
| 16 Pegasiπ | 0 | Anarchy | 19.19 | Yes | |
| Synuefai NU-D d13-49π | 0 | Anarchy | 20.91 | Yes | |
| Synuefai CA-G c27-14π | 0 | Anarchy | 21.42 | Yes | |
| Synuefai NU-D d13-55π | 0 | Anarchy | 21.57 | Yes | |
| Synuefai NU-D d13-63π | 0 | Anarchy | 22.18 | Yes | |
| Synuefai NB-K b55-3π | 0 | Anarchy | 24.67 | No | |
| Synuefai JV-L b54-2π | 0 | Anarchy | 26.24 | Yes | |
| Synuefai NU-D d13-41π | 0 | Anarchy | 26.51 | Yes | |
| Synuefai JV-L b54-1π | 0 | Anarchy | 26.84 | Yes | |
| Synuefai JV-L b54-3π | 0 | Anarchy | 27.22 | Yes | |
| Synuefai FP-N b53-3π | 0 | Anarchy | 27.95 | Yes | |
| Synuefai NU-D d13-65π | 0 | Anarchy | 31.77 | Yes | |
| Synuefai EP-N b53-3π | 0 | Anarchy | 31.80 | Yes | |
| Synuefai ZT-H c26-0π | 0 | Anarchy | 37.15 | No |