Overview
System: Mel 22 Sector NX-U d2-31 - All bodies
Distance to Sol: 465.17 ly
Spectral Class: F - Scoopable
Luminosity Class: Vb - Main-sequence star (dwarf)
Age: 1,200 Million years
Solar Masses: 1.1875
Solar Radius: 1.1545
Surface Temperature: 6,853 K
Absolute Magnitude: 3.7762
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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