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 |