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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Sifat Fisik

Kelas Spektral B Class B — B-type (Blue-White)
Indeks Warna (B−V) -0,118

Pengamatan

Magnitudo Semu +1.94
Magnitudo Mutlak -1,76
Jarak 179 ly

Posisi

Asensio Rekta 20h 25,65m
Deklinasi -56° 44,11′

Frequently Asked Questions

What type of star is Alpha Pavonis?
Alpha Pavonis is a Class B — B-type (Blue-White) star.
How far is Alpha Pavonis from Earth?
Alpha Pavonis is approximately 178.8 light-years from Earth.
Can you see Alpha Pavonis with the naked eye?
With an apparent magnitude of 1.94, Alpha Pavonis is visible to the naked eye.