System Byeia Euq YM-C b13-10 - E:D Companion

Byeia Euq YM-C b13-10

X: 591.625 / Y: 111.78125 / Z: 5616.28125
Updated
25d 21h
Minor faction ---
Allegiance None
Government None
Security Anarchy
Population 0
Primary None
Secondary None
Stellar Bodies 4
Stations 0
Fuel scoop Available
Byeia Euq YM-C b13-10 A M (Red dwarf) Star
Fuel scoop
Subclass9
LuminosityVI
Distance0.00ls
Stellar Mass0.23
Radius268,962,848.00
Absolute Magnitude11.29
Rotation Period126,634.04
Surface Temperature2102
Age12856
Axial Tilt0.00
Semi-Major Axis202,919,286,489.49
Eccentricity0.34
Orbital Inclination-8.75
Periapsis171.04
Orbital Period403,924,614.19
Ascending Node147.64
Mean Anomaly191.49
Byeia Euq YM-C b13-10 A 1 Sudarsky class III gas giant
Distance27.48ls
Ascending Node76.066119
Axial Tilt-0.514664
Eccentricity0.053671
Earth mass875.519836
Orbital Inclination30.087578
Orbital Period789264.625311
Periapsis32.206186
Radius71955280
Rotation Period793753.461876
Semi-Major Axis7874238491.0583
Surface Gravity67.398465
Surface Pressure0
Surface Temperature403.578552
Mean Anomaly147.606438
LandableNo
Tidal LockYes
Atmosphere Type---
Reserve Level---
Byeia Euq YM-C b13-10 B L (Brown dwarf) Star
Subclass6
LuminosityV
Distance2,597.95ls
Stellar Mass0.13
Radius205,627,536.00
Absolute Magnitude13.25
Rotation Period127,288.02
Surface Temperature1528
Age12856
Axial Tilt0.00
Semi-Major Axis378,400,188,684.46
Eccentricity0.34
Orbital Inclination-8.75
Periapsis351.04
Orbital Period403,924,614.19
Ascending Node147.64
Mean Anomaly191.49
Byeia Euq YM-C b13-10 C T (Brown dwarf) Star
Subclass1
LuminosityV
Distance158,925.81ls
Stellar Mass0.09
Radius139,639,104.00
Absolute Magnitude15.01
Rotation Period69,656.72
Surface Temperature1239
Age12856
Axial Tilt0.00
Semi-Major Axis34,876,679,182,052.61
Eccentricity0.10
Orbital Inclination47.49
Periapsis336.89
Orbital Period234,806,871,414.19
Ascending Node-56.93
Mean Anomaly207.65
System Minor faction Population Security Distance Scoopable
Byeia Euq SX-U d2-13 0 Anarchy 20.88 No
Byeia Euq RX-U d2-88 0 Anarchy 25.26 No