Bleae Thua BM-Y c11
X: -322.90625 / Y: 52.78125 / Z: 1537.375
Updated
49d 18h
49d 18h
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
Bleae Thua BM-Y c11 A
K (Yellow-Orange) Star
Fuel scoop
Subclass8
LuminosityVa
Distance0.00ls
Stellar Mass0.51
Radius486,667,456.00
Absolute Magnitude7.25
Rotation Period317,035.97
Surface Temperature3955
Age5754
Axial Tilt0.00
Semi-Major Axis1,190,954,864.03
Eccentricity0.09
Orbital Inclination-25.84
Periapsis19.85
Orbital Period187,154.60
Ascending Node101.17
Mean Anomaly111.00
Bleae Thua BM-Y c11 B
L (Brown dwarf) Star
Subclass2
LuminosityV
Distance15.05ls
Stellar Mass0.19
Radius235,024,144.00
Absolute Magnitude12.12
Rotation Period134,854.42
Surface Temperature1858
Age5754
Axial Tilt0.00
Semi-Major Axis3,159,675,657.75
Eccentricity0.09
Orbital Inclination-25.84
Periapsis199.85
Orbital Period187,154.60
Ascending Node101.17
Mean Anomaly111.00
Bleae Thua BM-Y c11 C
M (Red dwarf) Star
Fuel scoop
Subclass7
LuminosityVa
Distance5,731.44ls
Stellar Mass0.29
Radius293,286,720.00
Absolute Magnitude10.39
Rotation Period109,753.25
Surface Temperature2472
Age5754
Axial Tilt0.00
Semi-Major Axis4,001,684,248.45
Eccentricity0.30
Orbital Inclination-20.69
Periapsis3.92
Orbital Period949,456.18
Ascending Node-57.17
Mean Anomaly68.42
Bleae Thua BM-Y c11 D
M (Red dwarf) Star
Fuel scoop
Subclass9
LuminosityVI
Distance5,715.83ls
Stellar Mass0.16
Radius202,847,072.00
Absolute Magnitude12.03
Rotation Period80,755.70
Surface Temperature2040
Age5754
Axial Tilt0.00
Semi-Major Axis7,145,867,347.72
Eccentricity0.30
Orbital Inclination-20.69
Periapsis183.92
Orbital Period949,456.18
Ascending Node-57.17
Mean Anomaly68.42
| System | Minor faction | Population | Security | Distance | Scoopable |
|---|---|---|---|---|---|
| Bleae Thua XW-Y b3 | 0 | Anarchy | 17.70 | No | |
| Bleae Thua VB-Z b4 | 0 | Anarchy | 27.89 | Yes | |
| Bleae Thua VK-A c27 | 0 | Anarchy | 29.66 | No |