Overview
System: Wilatha Wang - All bodies
Distance to Sol: 114.72 ly
Spectral Class: F - Scoopable
Luminosity Class: Vb - Main-sequence star (dwarf)
Age: 4,216 Million years
Solar Masses: 1.3594
Solar Radius: 1.1322
Surface Temperature: 6,820 K
Orbital Period: 3,345,422.0 D
Semi Major Axis: 398.53 AU
Orbital Eccentricity: 0.0770
Orbital Inclination: -13.66 °
Arg Of Periapsis: 146.08 °
Absolute Magnitude: 3.8395
Materials:
None
Stations:
None

Class F stars are white main sequence stars. They range in mass from 1 to 1.4 solar masses and have a surface temperature reaching 7,600 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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