Overview
System: Heheng - All bodies
Distance to Sol: 106.73 ly
Spectral Class: F7 VI - Scoopable
Luminosity Class: VI - Subdwarf
Age: 1,716 Million years
Solar Masses: 1.0898
Solar Radius: 0.9752
Surface Temperature: 6,408 K
Orbital Period: 86,216.6 D
Semi Major Axis: 18.75 AU
Orbital Eccentricity: 0.0073
Orbital Inclination: 50.02 °
Arg Of Periapsis: 78.53 °
Absolute Magnitude: 4.4345
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.

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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