System: LTT 12360 - All bodies
Distance to Sol: 77.64 ly
Spectral Class: M - Scoopable
Distance To Arrival: 19,331 ls
Luminosity Class: V - Main-sequence star (dwarf)
Age: 8,030 Million years
Solar Masses: 0.3477
Solar Radius: 0.5084
Surface Temperature: 2,920 K
Orbital Period: 116,402.1 D
Semi Major Axis: 23.55 AU
Orbital Eccentricity: 0.2114
Orbital Inclination: 42.17 °
Arg Of Periapsis: 191.86 °
Absolute Magnitude: 9.2608

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.

LTT 12360 has missing or wrong info? Wanna help us to improve the data quality? Read the FAQ and Fix it on ROSS!