System Blae Drye GP-D d13-22 - E:D Companion

Blae Drye GP-D d13-22

X: -2567.65625 / Y: -296.53125 / Z: 5214.71875
Updated
51d 14h
Minor faction ---
Allegiance None
Government None
Security Anarchy
Population 0
Primary None
Secondary None
Stellar Bodies 4
Stations 0
Fuel scoop Available
Blae Drye GP-D d13-22 A F (White) Star
Fuel scoop
Subclass9
LuminosityVb
Distance0.00ls
Stellar Mass0.94
Radius732,495,040.00
Absolute Magnitude4.49
Rotation Period301,461.48
Surface Temperature6089
Age1052
Axial Tilt0.00
Semi-Major Axis17,551,085,352.90
Eccentricity0.03
Orbital Inclination-45.36
Periapsis61.10
Orbital Period2,721,809.39
Ascending Node36.06
Mean Anomaly224.63
Blae Drye GP-D d13-22 B G (White-Yellow) Star
Fuel scoop
Subclass7
LuminosityVab
Distance121.65ls
Stellar Mass0.90
Radius655,851,712.00
Absolute Magnitude5.28
Rotation Period296,521.63
Surface Temperature5368
Age1052
Axial Tilt0.00
Semi-Major Axis18,234,894,871.71
Eccentricity0.03
Orbital Inclination-45.36
Periapsis241.10
Orbital Period2,721,809.39
Ascending Node36.06
Mean Anomaly224.63
Blae Drye GP-D d13-22 C M (Red dwarf) Star
Fuel scoop
Subclass4
LuminosityVa
Distance24,394.23ls
Stellar Mass0.35
Radius391,919,136.00
Absolute Magnitude9.09
Rotation Period139,761.65
Surface Temperature2887
Age1052
Axial Tilt0.00
Semi-Major Axis352,947,127,819.06
Eccentricity0.10
Orbital Inclination18.06
Periapsis42.75
Orbital Period1,032,439,053.06
Ascending Node-100.09
Mean Anomaly109.16
Blae Drye GP-D d13-22 D L (Brown dwarf) Star
Subclass2
LuminosityV
Distance28,321.27ls
Stellar Mass0.14
Radius206,349,200.00
Absolute Magnitude12.51
Rotation Period94,503.82
Surface Temperature1812
Age1052
Axial Tilt0.00
Semi-Major Axis858,520,269,393.92
Eccentricity0.10
Orbital Inclination18.06
Periapsis222.75
Orbital Period1,032,439,053.06
Ascending Node-100.09
Mean Anomaly109.16
System Minor faction Population Security Distance Scoopable
Blae Drye EF-L b54-0 0 Anarchy 9.37 Yes
Blae Drye PP-F c27-14 0 Anarchy 18.80 Yes
Blae Drye DF-L b54-5 0 --- 19.21 No
Blae Drye WS-O b52-3 0 --- 29.94 No