Overview
System: Korovii - All bodies
Distance to Sol: 49.95 ly
Spectral Class: F - Scoopable
Luminosity Class: VI - Subdwarf
Age: 848 Million years
Solar Masses: 1.2656
Solar Radius: 1.1192
Surface Temperature: 7,242 K
Absolute Magnitude: 3.6038
Materials:
None
Stations:
None
Attractions: 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.

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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