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| physical object > naked eye object > naked eye star > Beta Trianguli |
| Beta Trianguli comparison table | |||||||||||||||||
| Subject | has right ascension | has declination | has spectral type | is part of | has surface temperature | is an instance of | has V magnitude | has color | has been observ | has B-V magnitude | has absorption line | is usually part of | is a kind of | has apparent magnitude | has synonym | has definition | has luminosity class |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| A star | O, B, A, and early F | 10000 K | white | H I | early star | Star with spectral type A in which the spectrum of the Balmer lines of hydrogen attain their greatest strength. Helium lines can no longer be seen. Some metallic lines are present; in late A stars the H and K lines of ionized calcium appear. A0 stars have a color index of zero. | |||||||||||
| bright giant | greater than 1000 Kelvin | star | II | ||||||||||||||
| 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 | ||||||||||
| Beta Trianguli | 2 9 32.5 | +34 59 14 | A5II | Milky Way | 10000 K | naked eye star | 3.00 | white | for many centuries | 0.14 | H I | asterism | brighter than 5 | HR 622 | II |
Next A star: Canum Venaticorum Up: A star, bright giant, naked eye star Previous A star: Ap star