NGC 2451A Sector HR-W d1-20
X: 656.75 / Y: -115.8125 / Z: -241.0625
Updated
14d 10h
14d 10h
System Governance
Minor faction ---
Allegiance None
Government None
Security Anarchy
Population 0
Economy & Assets
Primary None
Secondary None
Stellar Bodies 2
Stations 0
Fuel scoop
Available
NGC 2451A Sector HR-W d1-20
F (White) Star
Fuel scoop
Subclass8
LuminosityVab
Distance0.00ls
Stellar Mass1.29
Radius851,057,792.00
Absolute Magnitude4.11
Rotation Period395,269.10
Surface Temperature6169
Age664
Axial Tilt0.00
NGC 2451A Sector HR-W d1-20 5
High metal content body
Distance1,017.17ls
Ascending Node-138.391783
Axial Tilt0.522322
Eccentricity0.001897
Earth mass1.074722
Orbital Inclination0.123935
Orbital Period80658943.05706
Periapsis180.383957
Radius6214795
Rotation Period140943.605871
Semi-Major Axis304379546642.3
Surface Gravity11.090522
Surface Pressure316083.5
Surface Temperature214.957565
Mean Anomaly166.466331
LandableNo
Tidal LockNo
Atmosphere TypeNitrogen
Terraform StateTerraformable
Reserve Level---
| System | Minor faction | Population | Security | Distance | Scoopable |
|---|---|---|---|---|---|
| NGC 2451A Sector RE-Q b5-4 | 0 | Anarchy | 12.12 | No | |
| Synuefe NG-W c18-19 | 0 | Anarchy | 17.77 | No | |
| NGC 2451A Sector LD-S b4-4 | 0 | Anarchy | 20.76 | No | |
| NGC 2451A Sector PJ-Q b5-2 | 0 | Anarchy | 23.83 | Yes | |
| Synuefe GT-Q b38-1 | 0 | Anarchy | 23.98 | Yes | |
| Synuefe JZ-O b39-3 | 0 | Anarchy | 25.98 | No | |
| NGC 2451A Sector JC-V c2-7 | 0 | Anarchy | 26.02 | Yes | |
| Synuefe FT-Q b38-3 | 0 | --- | 26.89 | Yes | |
| Synuefe UA-L d9-58 | 0 | Anarchy | 27.02 | No | |
| Synuefe NG-W c18-2 | 0 | Anarchy | 28.01 | Yes | |
| Synuefe CY-Q b38-3 | 0 | --- | 28.21 | Yes | |
| NGC 2451A Sector PT-R b4-4 | 0 | Anarchy | 28.40 | Yes | |
| NGC 2451A Sector HR-W d1-106 | 0 | Anarchy | 28.62 | Yes | |
| Synuefe VA-L d9-64 | 0 | Anarchy | 29.77 | Yes | |
| Synuefe FJ-P b39-5 | 0 | Anarchy | 30.00 | No | |
| NGC 2451A Sector PT-R b4-5 | 0 | --- | 32.66 | Yes | |
| Synuefe JZ-O b39-0 | 0 | Anarchy | 33.71 | No |