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At apparent magnitude 1.94, Peacock is the brightest star of Pavo by Bayer designation, bearing the Alpha letter of that southern constellation. It belongs to the hot B spectral class, and its negative colour index of −0.118 confirms the blue-white cast expected of such high-temperature stars, whose surfaces are far warmer than the Sun's. Lying about 179 light-years distant, Peacock has an absolute magnitude of −1.76, marking it as intrinsically luminous — considerably brighter than its apparent rank alone would indicate. The gap of some 3.7 magnitudes between its apparent and absolute brightness is a direct expression of that distance. Its blue-white light and southerly position make Peacock a consistent naked-eye marker within the constellation of the same name.
물리적 특성
| 분광형 | B Class B — B-type (Blue-White) |
| 색지수 (B−V) | -0.118 |
관측
| 겉보기 등급 | +1.94 |
| 절대 등급 | -1.76 |
| 거리 | 179 ly |
위치
| 적경 | 20h 25.65m |
| 적위 | -56° 44.11′ |