System HIP 8664 - E:D Companion

HIP 8664

X: -73.1875 / Y: -493.8125 / Z: -222.0625
Updated
3d 16h
Minor faction ---
Allegiance None
Government None
Security Anarchy
Population 0
Primary None
Secondary None
Stellar Bodies 4
Stations 0
Fuel scoop Available
HIP 8664 A K (Yellow-Orange giant) Star
Subclass1
LuminosityIII
Distance0.00ls
Stellar Mass0.73
Radius10,161,371,136.00
Absolute Magnitude0.30
Rotation Period5,448,875.37
Surface Temperature4290
Age5580
Axial Tilt0.00
Semi-Major Axis10,363,473,296,165.47
Eccentricity0.14
Orbital Inclination-81.55
Periapsis357.18
Orbital Period103,944,927,454.00
Ascending Node-147.36
Mean Anomaly66.05
HIP 8664 B M (Red dwarf) Star
Fuel scoop
Subclass6
LuminosityVa
Distance108,010.87ls
Stellar Mass0.32
Radius327,989,536.00
Absolute Magnitude9.86
Rotation Period123,163.67
Surface Temperature2645
Age5580
Axial Tilt0.00
Semi-Major Axis23,349,027,633,666.99
Eccentricity0.14
Orbital Inclination-81.55
Periapsis177.18
Orbital Period103,944,927,454.00
Ascending Node-147.36
Mean Anomaly66.05
HIP 8664 C M (Red dwarf) Star
Fuel scoop
Subclass3
LuminosityVa
Distance439,147.83ls
Stellar Mass0.33
Radius359,593,504.00
Absolute Magnitude8.87
Rotation Period179,013.56
Surface Temperature3173
Age5580
Axial Tilt0.00
Semi-Major Axis1,397,532,165,050.51
Eccentricity0.05
Orbital Inclination6.32
Periapsis357.71
Orbital Period10,897,386,074.07
Ascending Node129.09
Mean Anomaly19.47
HIP 8664 D L (Brown dwarf) Star
Subclass9
LuminosityV
Distance456,051.42ls
Stellar Mass0.11
Radius161,097,552.00
Absolute Magnitude14.33
Rotation Period80,821.03
Surface Temperature1347
Age5580
Axial Tilt0.00
Semi-Major Axis4,192,596,614,360.81
Eccentricity0.05
Orbital Inclination6.32
Periapsis177.71
Orbital Period10,897,386,074.07
Ascending Node129.09
Mean Anomaly19.47
System Minor faction Population Security Distance Scoopable
HR 513 0 Anarchy 17.89 Yes
Synuefai PO-N b38-0 0 Anarchy 22.77 Yes
Synuefai RJ-N b38-0 0 Anarchy 24.70 Yes
HIP 8852 0 Anarchy 27.44 Yes
HIP 9352 0 Anarchy 33.66 No
Synuefai OO-N b38-0 0 Anarchy 34.02 No