System NGC 6193 Sector GW-W d1-14 - E:D Companion

NGC 6193 Sector GW-W d1-14

X: 1459.78125 / Y: -34.5625 / Z: 3422
Nearby search: Hotspots   |   Signals   |   Commodities
Updated
26d 5h
Minor faction ---
Allegiance None
Government None
Security Anarchy
Population 0
Primary None
Secondary None
Stellar Bodies 3
Stations 0
Fuel scoop Available
NGC 6193 Sector GW-W d1-14 A A (Blue-White) Star
Fuel scoop
Subclass9
LuminosityVab
Distance0.00ls
Stellar Mass1.70
Radius1,012,686,016.00
Absolute Magnitude2.76
Rotation Period80,721.97
Surface Temperature7707
Age780
Axial Tilt0.00
Semi-Major Axis3,116,917,490,959.17
Eccentricity0.22
Orbital Inclination-49.69
Periapsis198.83
Orbital Period18,126,127,123.83
Ascending Node-158.78
Mean Anomaly133.55
NGC 6193 Sector GW-W d1-14 A 1 Water world
Distance1,243.27ls
Ascending Node24.619045
Axial Tilt-0.255068
Eccentricity0.394589
Earth mass15.390852
Orbital Inclination-99.882019
Orbital Period130008685.58884
Periapsis336.54344
Radius19367848
Rotation Period77690.661328
Semi-Major Axis458792251348.5
Surface Gravity16.353447
Surface Pressure0
Surface Temperature239.618622
Mean Anomaly318.277185
LandableNo
Tidal LockNo
Atmosphere TypeNone
Reserve Level---
NGC 6193 Sector GW-W d1-14 B M (Red dwarf) Star
Fuel scoop
Subclass0
LuminosityVa
Distance52,759.05ls
Stellar Mass0.51
Radius490,997,312.00
Absolute Magnitude7.70
Rotation Period285,437.67
Surface Temperature3555
Age780
Axial Tilt0.00
Semi-Major Axis10,350,351,929,664.61
Eccentricity0.22
Orbital Inclination-49.69
Periapsis18.83
Orbital Period18,126,127,123.83
Ascending Node-158.78
Mean Anomaly133.55
System Minor faction Population Security Distance Scoopable
NGC 6193 Sector PA-J a11-1๐Ÿ“‹ 0 Anarchy 13.18 No
NGC 6193 Sector IO-M a9-0๐Ÿ“‹ 0 Anarchy 15.44 No
NGC 6193 Sector ER-V c2-6๐Ÿ“‹ 0 --- 18.54 Yes
NGC 6193 Sector MZ-K a10-1๐Ÿ“‹ 0 --- 20.07 No
NGC 6193 Sector FS-R b5-0๐Ÿ“‹ 0 Anarchy 25.17 Yes
NGC 6193 Sector SG-H a12-0๐Ÿ“‹ 0 --- 29.56 No
NGC 6193 Sector BM-T b4-1๐Ÿ“‹ 0 Anarchy 34.77 Yes
NGC 6193 Sector LY-P b6-2๐Ÿ“‹ 0 Anarchy 35.59 No