Peacock

Alp Pav

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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.

Physikalische Eigenschaften

Spektralklasse B Class B — B-type (Blue-White)
Farbindex (B−V) -0,118

Beobachtung

Scheinbare Helligkeit +1.94
Absolute Helligkeit -1,76
Entfernung 179 ly

Position

Rektaszension 20h 25,65m
Deklination -56° 44,11′

Frequently Asked Questions

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