Overview
System: HIP 23851 - All bodies
Distance to Sol: 343.34 ly
Spectral Class: G - Scoopable
Distance To Arrival: 238,530 ls
Luminosity Class: Vab - Main-sequence star (dwarf)
Age: 5,264 Million years
Solar Masses: 0.8828
Solar Radius: 0.9025
Surface Temperature: 5,431 K
Orbital Period: 2,438,259.7 D
Semi Major Axis: 342.28 AU
Orbital Eccentricity: 0.1907
Orbital Inclination: -53.75 °
Arg Of Periapsis: 99.10 °
Absolute Magnitude: 5.3212
Materials:
None
Stations:
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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