System Blae Drye YQ-O b25-2 - E:D Companion

Blae Drye YQ-O b25-2

X: -2136.09375 / Y: -217.84375 / Z: 4611.96875
Updated
4d 0h
Minor faction ---
Allegiance None
Government None
Security Anarchy
Population 0
Primary None
Secondary None
Stellar Bodies 4
Stations 0
Fuel scoop Available
Blae Drye YQ-O b25-2 A M (Red dwarf) Star
Fuel scoop
Subclass3
LuminosityVa
Distance0.00ls
Stellar Mass0.35
Radius363,838,496.00
Absolute Magnitude8.83
Rotation Period138,269.14
Surface Temperature3184
Age12892
Axial Tilt0.00
Semi-Major Axis3,331,410,765.65
Eccentricity0.08
Orbital Inclination-23.64
Periapsis160.34
Orbital Period442,148.45
Ascending Node93.04
Mean Anomaly166.73
Blae Drye YQ-O b25-2 B L (Brown dwarf) Star
Subclass1
LuminosityV
Distance27.29ls
Stellar Mass0.18
Radius254,444,976.00
Absolute Magnitude11.80
Rotation Period112,807.38
Surface Temperature1919
Age12892
Axial Tilt0.00
Semi-Major Axis444,797,980.79
Eccentricity0.03
Orbital Inclination13.62
Periapsis211.92
Orbital Period42,007.79
Ascending Node-108.22
Mean Anomaly198.82
Blae Drye YQ-O b25-2 C L (Brown dwarf) Star
Subclass8
LuminosityV
Distance26.26ls
Stellar Mass0.11
Radius180,900,448.00
Absolute Magnitude13.82
Rotation Period95,372.23
Surface Temperature1431
Age12892
Axial Tilt0.00
Semi-Major Axis741,330,325.60
Eccentricity0.03
Orbital Inclination13.62
Periapsis31.92
Orbital Period42,007.79
Ascending Node-108.22
Mean Anomaly198.82
Blae Drye YQ-O b25-2 D L (Brown dwarf) Star
Subclass9
LuminosityV
Distance4,201.24ls
Stellar Mass0.09
Radius161,224,896.00
Absolute Magnitude14.49
Rotation Period87,631.93
Surface Temperature1300
Age12892
Axial Tilt0.00
Semi-Major Axis1,032,319,366,931.92
Eccentricity0.11
Orbital Inclination50.22
Periapsis160.51
Orbital Period819,895,851.61
Ascending Node-26.21
Mean Anomaly129.42
System Minor faction Population Security Distance Scoopable
Blae Drye ES-M b26-3 0 Anarchy 23.19 Yes
Blae Drye XQ-O b25-6 0 Anarchy 26.89 No
Blae Drye WF-Q b24-5 0 Anarchy 26.90 Yes
Blae Drye ES-M b26-2 0 Anarchy 26.96 No
Blae Drye ZL-O b25-2 0 Anarchy 30.20 Yes