A Class K star is the sixth-brightest type of main sequence star. They are typically colored yellow-orange or orange. They make up roughly 12% of all main-sequence stars.
A typical Class K star has a mass of 0.6 (0.45 to 0.8) solar masses, a radius of 0.8 (0.7 to 0.96) solar radii, a luminosity of 0.3 (0.08 to 0.6) solar luminosities, a surface temperature of 4,450 K (3,700 K to 5,200 K), and a lifespan of 50 to 100 billion years.
With their extremely long lifespans and acceptable brightness, it is very likely that many Class K stars have life-bearing planets, and many exoplanets have been discovered around stars of this class.
Properties of K-type main sequence stars[]
Compared to stars like the Sun, K-type stars are generally notably smaller, cooler, less massive, and less luminous. Their small size and cooler temperatures are factors towards them being alternatively known as "orange dwarfs". The most luminous Class K stars are about two thirds the luminosity of the Sun while the least luminous are less than a tenth of the Sun's luminosity.
The spectra of Class K stars are characterized by strong sodium, neutral metal (e.g. Si I, Mn I, Fe I), and singly ionized metal (Ca II, Fe II) lines and extremely weak to nonexistent hydrogen lines. Lines of diatomic molecules such as TiO and CO are often present in cooler Class K stars.
Spectral type | Temperature (K) | Peak wavelength of black body of same temperature (nm) | Peak wavelength's light type | Chromaticity (D50) | Chromaticity (E) | Chromaticity (D65) | Colour index (B − V) | Mass (M⊙) | Radius (R⊙) | Luminosity (L⊙) | Apparent visual magnitude
(1 AU distance) |
Apparent visual magnitude
(1 pc distance) |
Absolute visual magnitude | Absolute bolometric magnitude | Examples |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
K0 V | 5230 | 554 | green | 0.819 | 0.81 | 0.817 | 0.468 | -25.67 | 0.90 | 5.90 | 5.54 | Sigma Draconis, 70 Ophiuchi A | |||
K1 V | 5080 | 570 | yellow | 0.866 | 0.79 | 0.814 | 0.437 | -25.47 | 1.10 | 6.10 | 5.65 | 107 Piscium | |||
K2 V | 4920 | 589 | orange/yellow | 0.912 | 0.76 | 0.763 | 0.337 | -25.17 | 1.40 | 6.40 | 5.88 | Epsilon Eridani | |||
K3 V | 4810 | 602 | orange | 0.966 | 0.74 | 0.729 | 0.263 | -24.87 | 1.70 | 6.70 | 6.16 | HD 219134 | |||
K4 V | 4640 | 625 | red/orange | 1.030 | 0.70 | 0.726 | 0.214 | -24.47 | 2.10 | 7.10 | 6.42 | TW Piscis Austrini | |||
K5 V | 4350 | 666 | red | 1.150 | 0.67 | 0.698 | 0.166 | -24.17 | 2.40 | 7.40 | 6.68 | 61 Cygni A | |||
K6 V | 4230 | 685 | red | 1.240 | 0.65 | 0.661 | 0.126 | -23.77 | 2.80 | 7.80 | 6.99 | HD 120467 | |||
K7 V | 4070 | 712 | red | 1.330 | 0.63 | 0.654 | 0.105 | -23.42 | 3.15 | 8.15 | 7.18 | 61 Cygni B | |||
K8 V | 4000 | 725 | red | 1.380 | 0.59 | 0.587 | 0.079 | -23.10 | 3.47 | 8.47 | 7.44 | HIP 111288 | |||
K9 V | 3940 | 736 | infrared/red | 1.420 | 0.56 | 0.552 | 0.066 | -22.88 | 3.69 | 8.69 | 7.59 | HIP 3261 |
See Also[]
Stellar Classes |
---|
Main sequence classes: L · M · K · G · F · A · B · O
Brown dwarf classes: Y · T · L · M |
Stellar Luminosity Classes |
---|
0 · I · II · III · IV · V · VI · VII |
References[]
- Cram, Lawrence E., and Leonard V. Kuhi. FGK Stars and T Tauri Stars. NASA, 1989.
- Mamajek, E., A Modern Mean Dwarf Stellar Color and Effective Temperature Sequence. 2019