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 |