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Peacock — Star in Pavo

HIP 100751; Alpha Pavonis

Magnitude 1.9m Star Pavo (Pav) Visible
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About Peacock

Description

Peacock is a blue-white star of spectral type B2IV at magnitude 1.94, the brightest star in Pavo (the Peacock). Located about 179 light-years from Earth, it has a luminosity of roughly 2,200 times solar and a surface temperature of about 17,700 K. It is a spectroscopic binary with an orbital period of about 11.75 days.

Observing Tips

Peacock is the brightest star in the southern constellation Pavo, visible from latitudes south of about 33°N. It lies in a relatively sparse area of sky south of Sagittarius. Its blue-white color is apparent to the naked eye. Best observed July through October from southern latitudes.

History

The name Peacock was assigned by Her Majesty's Nautical Almanac Office in the 1930s for navigational purposes — the star had no traditional name. Pavo was created by Petrus Plancius from Dutch navigators' observations in the late 16th century and represents the exotic peacock seen during voyages to the East Indies.

Fun Facts

Peacock is one of the brightest B-type stars visible from Earth and is the only star in Pavo bright enough to be used in celestial navigation. Like Avior in Carina, its name was specifically created for 20th-century navigators.

Observe

1Physical Properties

Magnitude 1.94
Spectral Type B3V
Star Color Blue (B-V -0.20)
Distance 179 ly

2Position & Identifiers

RA 20h 25m 38.9s
Dec -56° 44' 06.0"
Constellation Pavo (Pav)
HR 7790
HIP 100751
HD 193924
SAO 246574
Bayer Alpha

3How easy to spot?

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Equipment Bortle 3 Bortle 4 Bortle 5
Naked eye Easy Easy Easy
50mm finder Easy Easy Easy
150mm scope Easy Easy Easy
Easy Medium Hard Very hard Impossible

Bortle 3 = rural · 4 = outer suburbs · 5 = suburbs

4Visibility

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Best season Jun – Aug (peak: Jul)

5Survey Image

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Size Comparison

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Spectral Classification

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Hertzsprung-Russell Diagram

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Stellar Lifecycle

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Blackbody Spectrum

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Stellar Absorption Spectrum

Simulated absorption spectrum based on spectral type. Hover over lines to identify elements.

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Stellar Fusion

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15Stellar Notes

BC, 9.2, 10.2v sep. 17.6".
B0.5, B2, 11.753d, K 7.2k/s, V0 +2.0k/s, asini 1.16.
Color excess E(B-V) = +0.02.
Member of Pleiades group.
Lyman alpha and Lyman beta observed from COPERNICUS.
Peacock.
Diam. = 0.00077 - 0.00080".
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Light Travel Time Machine

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Relativistic Travel

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