|System:||Wredguia KL-W c15-6 - All bodies|
|Distance to Sol:||500.11 ly|
|Spectral Class:||K - Scoopable|
|Distance To Arrival:||4,934 ls|
|Luminosity Class:||Va - Main-sequence star (dwarf)|
|Age:||7,398 Million years|
|Surface Temperature:||3,960 K|
|Orbital Period:||8,757.2 D|
|Semi Major Axis:||4.73 AU|
|Orbital Inclination:||-37.50 °|
|Arg Of Periapsis:||69.29 °|
Class K stars are yellow-orange main sequence stars with a long and generally stable life. They range in mass from 0.6 to 0.9 solar masses and have a surface temperature reaching 5,000 K.
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.