알타이르 vs 베가
Two of the three corners of the Summer Triangle are A-type stars within 26 light-years of the Sun. Vega, at 25.04 light-years, shines at magnitude 0.03; Altair, closer at 16.73, manages only 0.76 — about half the light despite a 1.5-fold advantage in proximity. The reason sits in their absolute magnitudes, +0.60 for Vega and +2.21 for Altair, a gap of 1.61 magnitudes that makes Vega roughly four times the more luminous star. Altair is the nearer object; Vega is the stronger one, and in this pairing intrinsic output wins.
Property comparison
| Property | 알타이르 | 베가 |
|---|---|---|
| 명칭 | 53Alp Aql | 3Alp Lyr |
| 별자리 | Aquila | Lyra |
| 분광형 | Class A — A-type (White) | Class A — A-type (White) |
| 겉보기 등급 | +0.76 | +0.03 |
| 절대 등급 | 2.21 | 0.60 |
| 거리 | 16.7 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: 알타이르 · 베가
Key differences
Key Differences
- ◆ Both are A-type stars forming part of the Summer Triangle asterism along with Deneb.
- ◆ Vega is at 25 light-years; Altair is even closer at 16.7 light-years.
- ◆ Altair rotates extremely rapidly (once every 10.4 hours), making it noticeably oblate; Vega also rotates fast but less extremely.
- ◆ Vega is about four times more luminous than Altair.
- ◆ Vega has a prominent debris disk suggesting possible planetary formation; Altair's disk is less prominent.
When to Observe
알타이르
Vega culminates at midnight in late June and holds the summer evening sky through September. Its declination of +38° carries it close to the zenith for most of Europe and the northern United States.
베가
Altair follows about three weeks later, culminating at midnight in mid-July. At declination +8° it sits near the celestial equator and is accessible from both hemispheres.