Tr 24 Sector FW-V b31-2
X: 745.03125 / Y: -2.15625 / Z: 3765.8125
Updated
85d 3h
85d 3h
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
Tr 24 Sector FW-V b31-2 A
M (Red dwarf) Star
Fuel scoop
Subclass2
LuminosityVa
Distance0.00ls
Stellar Mass0.38
Radius399,581,376.00
Absolute Magnitude8.52
Rotation Period205,883.27
Surface Temperature3261
Age5582
Axial Tilt0.00
Semi-Major Axis733,927,685,022.35
Eccentricity0.07
Orbital Inclination-17.02
Periapsis278.69
Orbital Period2,016,292,572.02
Ascending Node14.11
Mean Anomaly279.37
Tr 24 Sector FW-V b31-2 A 1
Sudarsky class I gas giant
Distance259.20ls
Ascending Node-36.71171
Axial Tilt-0.189706
Eccentricity0.502063
Earth mass16.706287
Orbital Inclination-31.816353
Orbital Period36249986.886978
Periapsis257.624972
Radius21571604
Rotation Period178778.341397
Semi-Major Axis119151747226.72
Surface Gravity14.3095
Surface Pressure0
Surface Temperature132.207596
Mean Anomaly25.404075
LandableNo
Tidal LockNo
Atmosphere Type---
Reserve Level---
Tr 24 Sector FW-V b31-2 B
L (Brown dwarf) Star
Subclass0
LuminosityV
Distance6,584.56ls
Stellar Mass0.18
Radius249,520,800.00
Absolute Magnitude11.70
Rotation Period121,797.18
Surface Temperature1984
Age5582
Axial Tilt0.00
Semi-Major Axis33,450,653,553.01
Eccentricity0.00
Orbital Inclination-14.12
Periapsis114.29
Orbital Period81,941,610.57
Ascending Node107.70
Mean Anomaly332.07
Tr 24 Sector FW-V b31-2 C
T (Brown dwarf) Star
Subclass7
LuminosityV
Distance7,121.32ls
Stellar Mass0.04
Radius95,215,232.00
Absolute Magnitude17.47
Rotation Period44,648.20
Surface Temperature850
Age5582
Axial Tilt0.00
Semi-Major Axis136,843,585,968.02
Eccentricity0.00
Orbital Inclination-14.12
Periapsis294.29
Orbital Period81,941,610.57
Ascending Node107.70
Mean Anomaly332.07
| System | Minor faction | Population | Security | Distance | Scoopable |
|---|---|---|---|---|---|
| Tr 24 Sector DY-X c15-16📋 | 0 | --- | 12.56 | No |