Smojai IE-G b11-2
X: -54.03125 / Y: 115.03125 / Z: 3017.75
Updated
82d 18h
82d 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
Smojai IE-G b11-2 A
K (Yellow-Orange) Star
Fuel scoop
Subclass9
LuminosityVa
Distance0.00ls
Stellar Mass0.43
Radius446,764,480.00
Absolute Magnitude7.70
Rotation Period243,155.62
Surface Temperature3724
Age12902
Axial Tilt0.00
Semi-Major Axis2,339,198,589.32
Eccentricity0.21
Orbital Inclination26.16
Periapsis69.83
Orbital Period1,074,059.13
Ascending Node-113.12
Mean Anomaly58.70
Smojai IE-G b11-2 B
L (Brown dwarf) Star
Subclass8
LuminosityV
Distance39.43ls
Stellar Mass0.10
Radius168,377,728.00
Absolute Magnitude14.11
Rotation Period101,546.37
Surface Temperature1386
Age12902
Axial Tilt0.00
Semi-Major Axis10,386,043,787.00
Eccentricity0.21
Orbital Inclination26.16
Periapsis249.83
Orbital Period1,074,059.13
Ascending Node-113.12
Mean Anomaly58.70
Smojai IE-G b11-2 C
M (Red dwarf) Star
Fuel scoop
Subclass6
LuminosityVa
Distance425.59ls
Stellar Mass0.33
Radius373,877,920.00
Absolute Magnitude9.57
Rotation Period183,140.47
Surface Temperature2649
Age12902
Axial Tilt0.00
Semi-Major Axis74,115,282,297.13
Eccentricity0.13
Orbital Inclination-71.61
Periapsis164.51
Orbital Period24,532,631.64
Ascending Node65.97
Mean Anomaly101.55
Smojai IE-G b11-2 D
L (Brown dwarf) Star
Subclass4
LuminosityV
Distance47,775.25ls
Stellar Mass0.14
Radius194,378,304.00
Absolute Magnitude12.91
Rotation Period101,211.32
Surface Temperature1700
Age12902
Axial Tilt0.00
Semi-Major Axis11,995,759,606,361.39
Eccentricity0.08
Orbital Inclination-27.22
Periapsis64.16
Orbital Period28,468,632,698.06
Ascending Node55.82
Mean Anomaly256.38
| System | Minor faction | Population | Security | Distance | Scoopable |
|---|---|---|---|---|---|
| Smojai OT-R c4-7📋 | 0 | Anarchy | 6.74 | Yes | |
| Smojai OF-E b12-0📋 | 0 | Anarchy | 28.06 | Yes | |
| Smojai HT-H b10-3📋 | 0 | Anarchy | 30.58 | No |