System: Uzbekree - All bodies
Distance to Sol: 107.68 ly
Spectral Class: T - Not Scoopable
Distance To Arrival: 4,788 ls
Luminosity Class: V - Main-sequence star (dwarf)
Age: 5,194 Million years
Solar Masses: 0.0859
Solar Radius: 0.2142
Surface Temperature: 1,184 K
Orbital Period: 37,280.3 D
Semi Major Axis: 10.45 AU
Orbital Eccentricity: 0.5304
Orbital Inclination: 22.29 °
Arg Of Periapsis: 62.51 °
Absolute Magnitude: 15.0620

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.

Uzbekree B has missing or wrong info? Wanna help us to improve the data quality? Read the FAQ and Fix it on ROSS!