Drojeae IS-Q b52-0
X: -1423.53125 / Y: -104.625 / Z: 3900.09375
Updated
141d 2h
141d 2h
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
Drojeae IS-Q b52-0 A
M (Red dwarf) Star
Fuel scoop
Subclass0
LuminosityVa
Distance0.00ls
Stellar Mass0.44
Radius386,825,152.00
Absolute Magnitude8.21
Rotation Period186,708.38
Surface Temperature3561
Age4588
Axial Tilt0.00
Semi-Major Axis28,399,909,734,725.95
Eccentricity0.27
Orbital Inclination-49.84
Periapsis285.03
Orbital Period498,255,145,549.77
Drojeae IS-Q b52-0 B
M (Red dwarf) Star
Fuel scoop
Subclass9
LuminosityVI
Distance284,913.64ls
Stellar Mass0.17
Radius253,511,088.00
Absolute Magnitude11.60
Rotation Period133,843.60
Surface Temperature2013
Age4588
Axial Tilt0.00
Semi-Major Axis22,366,608,381.27
Eccentricity0.02
Orbital Inclination3.65
Periapsis144.02
Orbital Period29,642,458.56
Drojeae IS-Q b52-0 C
T (Brown dwarf) Star
Subclass3
LuminosityV
Distance284,841.42ls
Stellar Mass0.06
Radius127,816,800.00
Absolute Magnitude15.84
Rotation Period69,120.52
Surface Temperature1070
Age4588
Axial Tilt0.00
Semi-Major Axis65,608,738,660.81
Eccentricity0.02
Orbital Inclination3.65
Periapsis324.02
Orbital Period29,642,458.56
Drojeae IS-Q b52-0 BC 1
High metal content body
Distance291,217.68ls
Axial Tilt0.274638
Eccentricity0.015008
Earth mass6.197997
Orbital Inclination-45.932107
Orbital Period5440806448.4596
Periapsis229.15495
Radius10155773
Rotation Period106396.995026
Semi-Major Axis2841441333293.9
Surface Gravity23.951618
Surface Pressure14525.892578
Surface Temperature20.224615
LandableNo
Tidal LockNo
Atmosphere TypeHelium
Volcanismmajor silicate vapour geysers volcanism
Reserve Level---
| System | Minor faction | Population | Security | Distance | Scoopable |
|---|---|---|---|---|---|
| Drojeae FH-S b51-1📋 | 0 | Anarchy | 21.21 | Yes | |
| Drojeae NT-O b53-4📋 | 0 | Anarchy | 22.82 | Yes | |
| Drojeae EH-S b51-4📋 | 0 | Anarchy | 23.97 | No |