Overview
System: Wregoe TV-L c24-0 - All bodies
Distance to Sol: 1,214.84 ly
Spectral Class: M - Scoopable
Luminosity Class: Va - Main-sequence star (dwarf)
Age: 4,334 Million years
Solar Masses: 0.4648
Solar Radius: 0.6440
Surface Temperature: 3,369 K
Absolute Magnitude: 8.1284
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.

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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