| Subject | 
has right ascension | 
has spectral type | 
has declination | 
is part of | 
has surface temperature | 
has orbital period | 
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 | 
| G star |   | cooler than G2 |   |   | 5000 to 6000 K |   |   |   | yellowish |   |   |   |   | late star |   |   | Yellowish star in which the H and K lines of Ca II have become dominant and in which a tremendous profusion of spectral lines of both neutral and ionized metals, particularly iron, begins to show. The Balmer lines of hydrogen are still recognizable. Examples are the Sun and Capella. |   | 
| giant |   |   |   |   | greater than 1000 Kelvin |   |   |   |   |   |   |   |   | star |   |   | High-luminosity star that lies above the main sequence on the Hertzsprung-Russell diagram. | III | 
| 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 |   | 
| Capella | 05 16 41.3 | G5IIIe+G0III | +45 59 53 | Milky Way | 5000 to 6000 K | 104.023 days | naked eye star | 0.08 | yellowish | for many centuries | 0.80 | 13 pc | asterism |   | brighter than 5 | Alpha Aurigae | The sixth brightest star in the night sky, consists of two yellow giants. A spectroscopic triple (F8-G0 III, G5 III, M5 V) (1974 parallax 0'.079). It has a high lithium content and a nearly circular orbit. It may be an X-ray source. | III |