System Synuefe TH-G b54-0 - E:D Companion

Synuefe TH-G b54-0

X: 291.3125 / Y: -811 / Z: 106.0625
Updated
53d 10h
Minor faction ---
Allegiance None
Government None
Security Anarchy
Population 0
Primary None
Secondary None
Stellar Bodies 4
Stations 0
Fuel scoop Not available
Synuefe TH-G b54-0 A T Tauri Star
Subclass5
LuminosityVa
Distance0.00ls
Stellar Mass0.29
Radius343,632,352.00
Absolute Magnitude9.60
Rotation Period214,152.84
Surface Temperature2743
Age66
Axial Tilt0.00
Semi-Major Axis6,970,069,348.81
Eccentricity0.11
Orbital Inclination19.66
Periapsis266.31
Orbital Period3,182,803.63
Ascending Node-55.79
Mean Anomaly10.62
Synuefe TH-G b54-0 B T Tauri Star
Subclass4
LuminosityVI
Distance70.98ls
Stellar Mass0.12
Radius196,585,696.00
Absolute Magnitude12.96
Rotation Period107,850.10
Surface Temperature1674
Age66
Axial Tilt0.00
Semi-Major Axis16,960,508,823.39
Eccentricity0.11
Orbital Inclination19.66
Periapsis86.31
Orbital Period3,182,803.63
Ascending Node-55.79
Mean Anomaly10.62
Synuefe TH-G b54-0 AB 1 Sudarsky class I gas giant
Distance5,550.58ls
Ascending Node-48.446641
Axial Tilt0.436081
Eccentricity0.236536
Earth mass16.928656
Orbital Inclination98.977432
Orbital Period1537797152.9961
Periapsis77.506955
Radius21141886
Rotation Period47201.636315
Semi-Major Axis1473547816276.6
Surface Gravity15.095392
Surface Pressure0
Surface Temperature30.449797
Mean Anomaly249.124122
LandableNo
Tidal LockNo
Atmosphere Type---
Reserve Level---
Synuefe TH-G b54-0 C T Tauri Star
Subclass4
LuminosityVI
Distance97,312.06ls
Stellar Mass0.14
Radius217,025,376.00
Absolute Magnitude12.78
Rotation Period92,333.02
Surface Temperature1658
Age66
Axial Tilt0.00
Semi-Major Axis17,997,088,432,312.01
Eccentricity0.30
Orbital Inclination49.92
Periapsis104.90
Orbital Period87,939,453,125.00
Ascending Node-133.39
Mean Anomaly239.16
System Minor faction Population Security Distance Scoopable
Synuefe WD-D c27-3 0 Anarchy 6.21 Yes
Synuefe WD-D c27-2 0 Anarchy 8.52 Yes
Synuefe WL-C d13-15 0 Anarchy 14.24 Yes
Synuefe XD-D c27-0 0 Anarchy 17.54 No