Overview
System: Kotigen - All bodies
Distance to Sol: 167.21 ly
Spectral Class: M - Scoopable
Distance To Arrival: 16,062 ls
Luminosity Class: VI - Subdwarf
Age: 1,128 Million years
Solar Masses: 0.2266
Solar Radius: 0.3788
Surface Temperature: 2,139 K
Orbital Period: 68,940.5 D
Semi Major Axis: 21.91 AU
Orbital Eccentricity: 0.0841
Orbital Inclination: -23.43 °
Arg Of Periapsis: 45.05 °
Absolute Magnitude: 11.2546
Materials:
None
Stations:
None
Attractions: None

Class M stars are red stars that form the bulk of the main sequence stars in the galaxy. Their mass is low, as is their surface temperature.

A subdwarf, sometimes denoted by "sd", is a star with luminosity class VI under the Yerkes spectral classification system. They are defined as stars with luminosity 1.5 to 2 magnitudes lower than that of main-sequence stars of the same spectral type. On an Hertzsprung–Russell diagram subdwarfs appear to lie below the main sequence.

The term "subdwarf" was coined by Gerard Kuiper in 1939, to refer to a series of stars with anomalous spectra that were previously labeled as "intermediate white dwarfs".

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