| Subject | 
has right ascension | 
has spectral type | 
has declination | 
is part of | 
has surface temperature | 
is an instance of | 
has V magnitude | 
has color | 
has been observ | 
has B-V magnitude | 
has distance | 
is usually part of | 
is a kind of | 
has apparent magnitude | 
has synonym | 
has definition | 
has luminosity class | 
| giant |   |   |   |   | greater than 1000 Kelvin |   |   |   |   |   |   |   | star |   |   | High-luminosity star that lies above the main sequence on the Hertzsprung-Russell diagram. | III | 
| K star |   | cooler than G2 |   |   | 3600 to 5000 K |   |   | orange to red |   |   |   |   | late star |   |   | Cool star with spectral type K with spectra resembling those of sunspots, in which the hydrogen lines have been greatly weakened. The HK lines (q.v.) reach their greatest intensity. Strongest lines are Ca I (4227 Å) and the G-band (4303 Å). |   | 
| naked eye star |   |   |   | Milky Way | greater than 1000 Kelvin |   |   |   | for many centuries |   |   | asterism | naked eye object | brighter than 5 |   | A star visible without visual aids |   | 
| Aldebaran | 4 35 55.2 | K5III | +16 30 33 | Milky Way | 3600 to 5000 K | naked eye star | 0.85 | orange to red | for many centuries | 1.54 | 21 parsecs | asterism |   | brighter than 5 | HR 1457 | A K5 III subgiant (a foreground star in the Hyades). It has a faint M2 V companion. It is now known to be slowly and irregularly variable. | III |