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 |
is usually part of |
is a kind of |
has apparent magnitude |
has synonym |
has definition |
has luminosity class |
bright giant | | | | | greater than 1000 Kelvin | | | | | | | star | | | | II |
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 | |
Arcturus | 14 15 39.6 | K1IIIbCN-1 | +19 10 57 | Milky Way | 3600 to 5000 K | naked eye star | -0.04 | orange to red | for many centuries | 1.23 | asterism | | brighter than 5 | HR 5340 | An old subgiant disk star (K2 IIIp, mv = 0.06) about 11 pc distant. | II |