Hegeia AF-A b55-2
X: -2098.375 / Y: 11.03125 / Z: -2426.4375
Updated
17d 1h
17d 1h
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
Hegeia AF-A b55-2 A
M (Red dwarf) Star
Fuel scoop
Subclass3
LuminosityVa
Distance0.00ls
Stellar Mass0.44
Radius397,034,368.00
Absolute Magnitude8.69
Rotation Period169,267.32
Surface Temperature3147
Age8606
Axial Tilt0.00
Semi-Major Axis63,593,050,837.52
Eccentricity0.11
Orbital Inclination62.43
Periapsis221.63
Orbital Period26,096,477.51
Ascending Node50.29
Mean Anomaly238.71
Hegeia AF-A b55-2 B
M (Red dwarf) Star
Fuel scoop
Subclass8
LuminosityVa
Distance450.51ls
Stellar Mass0.25
Radius265,588,096.00
Absolute Magnitude10.95
Rotation Period116,346.10
Surface Temperature2288
Age8606
Axial Tilt0.00
Semi-Major Axis544,742,655.75
Eccentricity0.04
Orbital Inclination30.23
Periapsis202.38
Orbital Period35,771.35
Ascending Node63.55
Mean Anomaly154.59
Hegeia AF-A b55-2 C
M (Red dwarf) Star
Fuel scoop
Subclass8
LuminosityVa
Distance446.91ls
Stellar Mass0.20
Radius258,286,720.00
Absolute Magnitude11.21
Rotation Period112,623.27
Surface Temperature2184
Age8606
Axial Tilt0.00
Semi-Major Axis697,270,870.21
Eccentricity0.04
Orbital Inclination30.23
Periapsis22.38
Orbital Period35,771.35
Ascending Node63.55
Mean Anomaly154.59
Hegeia AF-A b55-2 D
M (Red dwarf) Star
Fuel scoop
Subclass6
LuminosityVa
Distance11,795.04ls
Stellar Mass0.30
Radius350,933,728.00
Absolute Magnitude9.85
Rotation Period162,080.71
Surface Temperature2563
Age8606
Axial Tilt0.00
Semi-Major Axis2,738,018,631,935.12
Eccentricity0.05
Orbital Inclination17.86
Periapsis196.48
Orbital Period3,525,448,501.11
Ascending Node-60.09
Mean Anomaly24.58
| System | Minor faction | Population | Security | Distance | Scoopable |
|---|---|---|---|---|---|
| Hegeia KI-B d13-17📋 | 0 | Anarchy | 15.83 | Yes | |
| Hegeia OO-Z d13-8📋 | 0 | Anarchy | 24.02 | Yes | |
| Hegeia KI-B d13-2📋 | 0 | Anarchy | 27.95 | No |