HIP 65032
X: 371.1875 / Y: 250.8125 / Z: 312.6875
Updated
10d 3h
10d 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
HIP 65032
F (White) Star
Fuel scoop
Subclass2
LuminosityV
Distance0.00ls
Stellar Mass1.39
Radius856,894,656.00
Absolute Magnitude3.25
Rotation Period222,553.31
Surface Temperature6973
Age634
Axial Tilt0.00
HIP 65032 1
Metal rich body
Landable
Distance14.75ls
Ascending Node-84.715755
Axial Tilt-0.001284
Eccentricity6.2E-5
Earth mass0.613855
Orbital Inclination-0.00032
Orbital Period133759.796619
Periapsis345.08776
Radius5126892.5
Rotation Period135940.795178
Semi-Major Axis4420967757.7019
Surface Gravity9.308223
Surface Pressure0
Surface Temperature2095.100098
Mean Anomaly341.721896
LandableYes
Tidal LockYes
Atmosphere TypeNone
Volcanismmajor metallic magma volcanism
Reserve Level---
Iron39.57%
Nickel29.93%
Chromium17.80%
Zirconium4.59%
Cadmium3.07%
Tungsten2.17%
Antimony1.47%
Selenium1.39%
HIP 65032 8
Y (Brown dwarf) Star
Subclass5
LuminosityV
Distance6,407.77ls
Stellar Mass0.01
Radius39,138,852.00
Absolute Magnitude22.68
Rotation Period77,799.93
Surface Temperature330
Age634
Axial Tilt-0.03
Semi-Major Axis1,899,336,993,694.31
Eccentricity0.02
Orbital Inclination-1.69
Periapsis46.57
Orbital Period1,191,112,041.47
Ascending Node-80.40
Mean Anomaly231.59
HIP 65032 9
Y (Brown dwarf) Star
Subclass3
LuminosityV
Distance9,137.41ls
Stellar Mass0.02
Radius55,970,260.00
Absolute Magnitude21.38
Rotation Period402,824.07
Surface Temperature444
Age634
Axial Tilt1.86
Semi-Major Axis2,651,713,192,462.92
Eccentricity0.05
Orbital Inclination-4.32
Periapsis64.34
Orbital Period1,964,895,248.41
Ascending Node153.08
Mean Anomaly128.35
| System | Minor faction | Population | Security | Distance | Scoopable |
|---|---|---|---|---|---|
| Praea Euq DV-Y d44 | 0 | Anarchy | 16.31 | No | |
| HIP 64859 | 0 | Anarchy | 22.21 | Yes | |
| Praea Euq EV-X c1-10 | 0 | Anarchy | 32.82 | No |