System: Neritus - All bodies
Distance to Sol: 81.55 ly
Spectral Class: G - Scoopable
Luminosity Class: V - Main-sequence star (dwarf)
Age: 888 Million years
Solar Masses: 1.0312
Solar Radius: 1.0350
Surface Temperature: 5,846 K
Orbital Period: 21,440.2 D
Semi Major Axis: 4.74 AU
Orbital Eccentricity: 0.1537
Orbital Inclination: 0.94 °
Arg Of Periapsis: 45.16 °
Absolute Magnitude: 4.9707
Gliese ID: GL 925
HIP ID: 39,710
HD ID: 67,458
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.