くじゃく座アルファ星

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.

物理的特性

スペクトル型 B Class B — B-type (Blue-White)
色指数 (B−V) -0.118

観測

見かけの等級 +1.94
絶対等級 -1.76
距離 179 ly

位置

赤経 20h 25.65m
赤緯 -56° 44.11′

Frequently Asked Questions

What type of star is くじゃく座アルファ星?
くじゃく座アルファ星 is a Class B — B-type (Blue-White) star.
How far is くじゃく座アルファ星 from Earth?
くじゃく座アルファ星 is approximately 178.8 light-years from Earth.
Can you see くじゃく座アルファ星 with the naked eye?
With an apparent magnitude of 1.94, くじゃく座アルファ星 is visible to the naked eye.