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Zhenruj (Mu Herculis)

Part of the pre-Nexus Vega wormhole network

Mu Herculis System
Image from Steve Bowers
The Zhenruj system has four stars, but no major planets. The luminosity of the stars in this system is collected by power swarms and beamed to the Oort Cloud, providing energy to various godtech nodes and other structures. Zhenruj was one of the first four stars connected to Aksijaha by wormhole, before the expansion of the Wormhole Nexus. This system is almost exclusively reserved for transapient use, but has a small population of devout god-dwellers

Zhenruj System - Data Panel

SystemNames: Zhenruj
Components: 4
1) Mademgo (Mu Herculis Aa)
2) Horbo (Mu Herculis Ab)
3) Maazhti (Mu Herculis B)
4) Byoktu (Mu Herculis C)
Location:
- Distance from Aksijaha: 7.259 ly (J2000)
- Distance from Sol: 27.20 ly (J2000)
- Constellation: Hercules
MademgoNames: Mademgo, Mu Herculis Aa, Mu1 Herculis A, 86 Herculis A, Gliese 695 Aa (GJ 695 Aa), HD 161797, HIP 86974, HR 6623
Physical characteristics:
- Mass: 1.11 x Sol
- Radius: 1.704 x Sol
- Temperature: 5,596 Kelvin
- Luminosity: 2.557 x Sol (bolometric)
- Spectral type: G5 IV
- Rotation period: 52 days
- Age: 7.480 billion years
HorboNames: Horbo, Mu Herculis Ab, Mu1 Herculis B, 86 Herculis B, Gliese 695 Ab (GJ 695 Ab)
Physical characteristics:
- Mass: 0.2214 x Sol
- Spectral type: M4 V
- Age: 7.480 billion years
Mu1 Herculis binary orbitOrbital characteristics:
- Average separation: 20.5 AU
- Orbital period: 81.610 years
- Eccentricity: 0.386
MaazhtiNames: Maazhti, Mu Herculis B, Mu2 Herculis A, Gliese 695 B (GJ 695 B)
Physical characteristics:
- Mass: 0.44 x Sol
- Radius: 0.423 x Sol
- Temperature: 3,345 Kelvin
- Luminosity: 0.0202 x Sol (bolometric)
- Spectral type: M3.7 V
- Age: 7.480 billion years
ByoktuNames: Byoktu, Mu Herculis C, Mu2 Herculis B, Gliese 695 C (GJ 695 C)
Physical characteristics:
- Mass: 0.39 x Sol
- Radius: 0.273 x Sol
- Temperature: 3,100 Kelvin
- Luminosity: 0.0062 x Sol (bolometric)
- Spectral type: M4.7 V
- Age: 7.480 billion years
Mu2 Herculis binary orbitOrbital characteristics:
- Average separation: 11.5 AU
- Orbital period: 43.127 years
- Eccentricity: 0.1796
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Development Notes
Text by The Astronomer (2021)
Original article by Anders Sandberg
Initially published on 08 December 2001.

 
 
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