альфа Павлина

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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Физические свойства

Спектральный класс B Class B — B-type (Blue-White)
Показатель цвета (B−V) -0,118

Наблюдение

Видимая звёздная величина +1.94
Абсолютная звёздная величина -1,76
Расстояние 179 ly

Положение

Прямое восхождение 20h 25,65m
Склонение -56° 44,11′

Frequently Asked Questions

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