Фомальгаут vs Вега
A gap of 1.14 magnitudes puts Вега clearly ahead overhead, +0.03 to +1.17. Both lie at a comparable distance from the Sun — 25.1 light-years for Фомальгаут and 25.0 for Вега. Intrinsically the balance shifts: Вега carries an absolute magnitude of +0.60 against +1.74 for Фомальгаут, making it about 2.9 times more luminous once distance is removed from the comparison. By spectral type the pair divides into an A-type star for Фомальгаут and an A-type star in Lyra for Вега.
Property comparison
| Property | Фомальгаут | Вега |
|---|---|---|
| Обозначение | 24Alp PsA | 3Alp Lyr |
| Созвездие | N/A | Lyra |
| Спектральный класс | Class A — A-type (White) | Class A — A-type (White) |
| Видимая звёздная величина | +1.17 | +0.03 |
| Абсолютная звёздная величина | 1.74 | 0.60 |
| Расстояние | 25.1 ly | 25.0 ly |
| Масса | N/A | N/A |
| Радиус | N/A | N/A |
| Температура | N/A | N/A |
| Светимость | N/A | N/A |
Full data for each star: Фомальгаут · Вега
Key differences
Key Differences
- ◆ Both are young A-type benchmark stars with prominent debris disks, used to calibrate stellar and planetary evolution models.
- ◆ Fomalhaut is the southernmost autumn star easily seen from northern mid-latitudes.
- ◆ Vega is approximately 1.9 times more massive than Fomalhaut.
- ◆ Both have been candidate targets for direct imaging of orbiting companions.
- ◆ Fomalhaut is one of only 18 stars with disks resolved by Hubble; Vega's disk was first revealed by IRAS in 1983.