Overview
System: Pleiades Sector IM-V c2-16 - All bodies
Distance to Sol: 343.90 ly
Spectral Class: T - Not Scoopable
Distance To Arrival: 420 ls
Luminosity Class: V - Main-sequence star (dwarf)
Age: 5,714 Million years
Solar Masses: 0.0469
Solar Radius: 0.1487
Surface Temperature: 765 K
Orbital Period: 0.5 D
Semi Major Axis: 0.01 AU
Orbital Eccentricity: 0.0326
Orbital Inclination: -19.50 °
Arg Of Periapsis: 181.53 °
Absolute Magnitude: 17.7517
Materials:
None
Stations:
None

Class T dwarfs are brown dwarfs with a surface temperature between 700 and 1,300 K. They are sometimes known as Methane Dwarfs due to the prominence of methane in their composition. They are on the borderline between what might be considered a very large gas giant planet and a star.

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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