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Suhail Hadar — Star in Puppis

HIP 39429; Zeta Puppis

Magnitude 2.2m Star Puppis (Pup) Visible
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About Suhail Hadar

Description

Naos (also known as Suhail Hadar) is one of the hottest and most luminous stars visible to the naked eye. At spectral type O5Iaf and magnitude 2.25, it is a blue supergiant with a surface temperature of about 42,000 K and a luminosity roughly 800,000 times that of the Sun. Located approximately 1,080 light-years away, Naos has a powerful stellar wind that ejects mass at a rate millions of times greater than the Sun's solar wind.

Observing Tips

Located in the southeastern part of Puppis, Naos is a striking blue-white star best viewed from the southern hemisphere or from low northern latitudes. It sits in a rich part of the Milky Way with many background stars. Binoculars reveal its vivid blue-white color against the star-rich backdrop. Best observed from January through April. From northern mid-latitudes it is low on the southern horizon.

History

The name Naos comes from the Greek 'naos,' meaning 'ship,' referring to the constellation Puppis (the stern of the mythological ship Argo). The alternate name Suhail Hadar is Arabic in origin. Zeta Pup was one of the first stars whose extreme temperature was determined spectroscopically, revealing it as an O-type supergiant — among the most massive and energetic stars known.

Fun Facts

Naos is a stellar powerhouse — if placed where the Sun is, it would appear 16,700 times brighter and would completely sterilize all planets in the solar system with its intense ultraviolet radiation. It is also a runaway star, hurtling through space at an unusually high velocity, likely ejected from a binary system when its companion exploded as a supernova.

Observe

1Physical Properties

Magnitude 2.25
Range 2.24 - 2.26
Period 42.7 hours
Variable Type ROT:
Spectral Type O6/7III
Star Color Blue (B-V -0.26)
Distance 1,082 ly

2Position & Identifiers

RA 08h 03m 35.1s
Dec -40° 00' 12.0"
Constellation Puppis (Pup)
HR 3165
HIP 39429
HD 66811
SAO 198752
Bayer Zeta

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 Dec – Feb (peak: Jan)

5Survey Image

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Explore

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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

Change in H alpha emission profile between 1974 and 1976 interpreted as change in rate of mass loss.
Color excess E(B-V) = +0.04.
In cluster CR 173; in HII region.
Also classified O4f, O4ef and O4I9n)f.
Naos; Suhail Hadar.
Diam. = 0.00041 - 0.00042".
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Light Travel Time Machine

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Relativistic Travel

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