K-type main-sequence star
| K-type main-sequence star | |
|---|---|
Sigma Draconis, officially named Alsafi, is a K-type main-sequence star. | |
| Characteristics | |
| Type | Class of medium-small main sequence star |
| Mass range | 0.60–0.86 M☉ |
| Temperature | 3,930–5,270 K |
| Average luminosity | 0.079–0.47 L☉ |
| External links | |
| Media category | |
| Q863936 | |
A K-type main-sequence star is a main-sequence (core hydrogen-burning) star of spectral type K. The spectral luminosity class is V. These stars are intermediate in size between red dwarfs and yellow dwarfs, hence the term orange dwarfs often applied to this type.