Byoomi TG-X b21-41
X: -1594.8125 / Y: -51.46875 / Z: 25001.6875
Updated
108d 12h
108d 12h
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
Byoomi TG-X b21-41 A
M (Red dwarf) Star
Fuel scoop
Subclass9
LuminosityVI
Distance0.00ls
Stellar Mass0.23
Radius264,017,456.00
Absolute Magnitude11.24
Rotation Period98,234.42
Surface Temperature2144
Age3646
Axial Tilt0.00
Semi-Major Axis1,605,185,329.91
Eccentricity0.00
Orbital Inclination28.87
Periapsis137.48
Orbital Period364,019.77
Ascending Node82.12
Mean Anomaly275.85
Byoomi TG-X b21-41 B
L (Brown dwarf) Star
Subclass8
LuminosityV
Distance17.71ls
Stellar Mass0.10
Radius150,803,440.00
Absolute Magnitude14.28
Rotation Period72,864.09
Surface Temperature1409
Age3646
Axial Tilt0.00
Semi-Major Axis3,704,274,594.78
Eccentricity0.00
Orbital Inclination28.87
Periapsis317.48
Orbital Period364,019.77
Ascending Node82.12
Mean Anomaly275.85
Byoomi TG-X b21-41 C
L (Brown dwarf) Star
Subclass3
LuminosityV
Distance2,667.47ls
Stellar Mass0.15
Radius205,096,912.00
Absolute Magnitude12.71
Rotation Period99,861.92
Surface Temperature1734
Age3646
Axial Tilt0.00
Semi-Major Axis565,796,566,009.52
Eccentricity0.09
Orbital Inclination-16.69
Periapsis264.06
Orbital Period577,389,597.89
Ascending Node-132.69
Mean Anomaly70.64
Byoomi TG-X b21-41 D
L (Brown dwarf) Star
Subclass8
LuminosityV
Distance71,267.99ls
Stellar Mass0.12
Radius168,335,264.00
Absolute Magnitude14.02
Rotation Period77,197.85
Surface Temperature1417
Age3646
Axial Tilt0.00
Semi-Major Axis12,519,068,121,910.10
Eccentricity0.40
Orbital Inclination5.11
Periapsis105.14
Orbital Period43,106,345,534.32
Ascending Node-63.18
Mean Anomaly145.45
| System | Minor faction | Population | Security | Distance | Scoopable |
|---|---|---|---|---|---|
| Byoomi HN-M c10-1707📋 | 0 | Anarchy | 12.58 | Yes | |
| Byoomi XM-V b22-150📋 | 0 | Anarchy | 16.72 | Yes | |
| Byoomi AV-X e1-6811📋 | 0 | Anarchy | 27.22 | No |