System HIP 20942 - E:D Companion

HIP 20942

X: 225.9375 / Y: -436.25 / Z: -640.65625
Updated
1562d 15h
Minor faction ---
Allegiance None
Government None
Security Anarchy
Population 0
Primary None
Secondary None
Stellar Bodies 5
Stations 0
Fuel scoop Available
HIP 20942 A (Blue-White) Star
Fuel scoop
Subclass2
LuminosityV
Distance0.00ls
Stellar Mass2.04
Radius1,091,600,384.00
Absolute Magnitude1.99
Rotation Period52,753.39
Surface Temperature9155
Age1064
Axial Tilt0.00
HIP 20942 7 Y (Brown dwarf) Star
Subclass5
LuminosityV
Distance1,264.59ls
Stellar Mass0.01
Radius39,202,528.00
Absolute Magnitude23.42
Rotation Period54,451.62
Surface Temperature342
Age1064
Axial Tilt1.90
Semi-Major Axis16,157,629.49
Eccentricity0.19
Orbital Inclination4.19
Periapsis189.76
Orbital Period9,416,111.59
HIP 20942 10 Y (Brown dwarf) Star
Subclass5
LuminosityV
Distance2,180.30ls
Stellar Mass0.01
Radius47,013,316.00
Absolute Magnitude23.35
Rotation Period85,459.03
Surface Temperature331
Age1064
Axial Tilt0.14
Semi-Major Axis16,909,271,478.65
Eccentricity0.18
Orbital Inclination0.30
Periapsis121.75
Orbital Period9,036,856.95
HIP 20942 11 Y (Brown dwarf) Star
Subclass0
LuminosityV
Distance2,210.87ls
Stellar Mass0.03
Radius77,980,560.00
Absolute Magnitude19.29
Rotation Period88,422.96
Surface Temperature689
Age1064
Axial Tilt-0.82
Semi-Major Axis7,150,359,749.79
Eccentricity0.18
Orbital Inclination0.30
Periapsis301.75
Orbital Period9,036,856.95
HIP 20942 12 Y (Brown dwarf) Star
Subclass1
LuminosityV
Distance4,100.63ls
Stellar Mass0.03
Radius76,133,984.00
Absolute Magnitude19.78
Rotation Period75,020.96
Surface Temperature599
Age1064
Axial Tilt-2.09
Semi-Major Axis1,226,020,991,802.22
Eccentricity0.00
Orbital Inclination1.70
Periapsis180.45
Orbital Period505,371,749.40
System Minor faction Population Security Distance Scoopable
Synuefe FJ-M c9-1 0 Anarchy 14.51 No
Synuefe ND-X b19-0 0 Anarchy 15.24 No
Synuefe PO-V b20-0 0 --- 23.79 Yes
Synuefe JX-Y b18-0 0 --- 23.81 Yes
Synuefe DO-M c9-0 0 Anarchy 25.34 Yes
Synuefe LI-X b19-0 0 Anarchy 30.54 Yes