Alpha Pavonis
Alp Pav
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.
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Propriedades físicas
| Classe Espectral | B Class B — B-type (Blue-White) |
| Índice de cor (B−V) | -0,118 |
Observação
| Magnitude Aparente | +1.94 |
| Magnitude Absoluta | -1,76 |
| Distância | 179 ly |
Posição
| Ascensão reta | 20h 25,65m |
| Declinação | -56° 44,11′ |