Overview
System: 108 Herculis - All bodies
Distance to Sol: 183.22 ly
Spectral Class: G7 Vab - Scoopable
Distance To Arrival: 922 ls
Luminosity Class: Vab - Main-sequence star (dwarf)
Age: 1,186 Million years
Solar Masses: 0.8516
Solar Radius: 0.9752
Surface Temperature: 5,408 K
Orbital Period: 504.8 D
Semi Major Axis: 1.29 AU
Orbital Eccentricity: 0.0733
Orbital Inclination: 26.93 °
Arg Of Periapsis: 152.94 °
Absolute Magnitude: 5.1714
HIP ID: 89925
HD ID: 168913
Materials:
None
Stations:
None
Attractions: None

Class G stars are white-yellow main sequence stars. They range in mass from 0.8 to 1.2 solar masses and have a surface temperature reaching 6,000 K.

The term dwarf star refers to a variety of distinct classes of stars. The term was originally coined in 1906 when the Danish astronomer Ejnar Hertzsprung noticed that the reddest stars - classified as K and M in the Harvard scheme - could be divided into two distinct groups. They are either much brighter than the Sun, or much fainter. To distinguish these groups, he called them "giant" and "dwarf" stars, the dwarf stars being fainter and the giants being brighter than the sun.

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