Rigel
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Rigel's absolute magnitude of −6.93 ranks it among the most intrinsically luminous stars on StarFYI, a beacon whose light travels 863 years to reach Earth yet still arrives at apparent magnitude 0.18. Designated Beta Orionis, it marks the bright foot of the constellation Orion and shows the blue-white colour of a B-type star, corroborated by a B–V index of −0.03. Its position near the celestial equator, at declination −8°, renders it visible from virtually every inhabited region of the planet. The sheer distance over which Rigel remains a first-magnitude star underscores an output thousands of times greater than the Sun's — the defining trait of the sky's most remote brilliant stars.
物理特性
| 光谱类型 | B Class B — B-type (Blue-White) |
| 色指数 (B−V) | -0.030 |
观测
| 视星等 | +0.18 |
| 绝对星等 | -6.93 |
| 距离 | 863 ly |
| 星座 | Orion |
位置
| 赤经 | 5h 14.54m |
| 赤纬 | -8° 12.10′ |
Related Chemistry
Explore the chemical elements connected to Rigel on our sister site ChemFYI.
Hydrogen Balmer series visible in B-type supergiants
Neutral helium lines are a defining feature of B-type spectra
CNO-cycle product enriched in blue supergiant atmospheres
Part of the Science FYI Family