포말하우트 vs 베가
A gap of 1.14 magnitudes puts 베가 clearly ahead overhead, +0.03 to +1.17. Both lie at a comparable distance from the Sun — 25.1 light-years for 포말하우트 and 25.0 for 베가. Intrinsically the balance shifts: 베가 carries an absolute magnitude of +0.60 against +1.74 for 포말하우트, 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 포말하우트 and an A-type star in Lyra for 베가.
Property comparison
| Property | 포말하우트 | 베가 |
|---|---|---|
| 명칭 | 24Alp PsA | 3Alp Lyr |
| 별자리 | N/A | Lyra |
| 분광형 | Class A — A-type (White) | Class A — A-type (White) |
| 겉보기 등급 | +1.17 | +0.03 |
| 절대 등급 | 1.74 | 0.60 |
| 거리 | 25.1 ly | 25.0 ly |
| 질량 | N/A | N/A |
| 반지름 | N/A | N/A |
| 온도 | N/A | N/A |
| 광도 | N/A | N/A |
Full data for each star: 포말하우트 · 베가
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.