Overview
System: Pleiades Sector IR-W d1-64 - All bodies
Distance to Sol: 341.47 ly
Spectral Class: M - Scoopable
Distance To Arrival: 3,140 ls
Luminosity Class: Va - Main-sequence star (dwarf)
Age: 396 Million years
Solar Masses: 0.2852
Solar Radius: 0.4684
Surface Temperature: 2,525 K
Orbital Period: 5,180.6 D
Semi Major Axis: 4.18 AU
Orbital Eccentricity: 0.0820
Orbital Inclination: -72.49 °
Arg Of Periapsis: 84.62 °
Absolute Magnitude: 10.0727
Materials:
None
Stations:
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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