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Saiph — Star in Orion

HIP 27366; Kappa Orionis; 53 Orionis

Magnitude 2.1m Star Orion (Ori) Visible
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About Saiph

Description

Saiph marks the southeastern foot of Orion and is a blue supergiant of spectral type B0.5Ia at magnitude 2.06. Despite appearing similar in brightness to Rigel (Orion's other foot), Saiph is actually much farther away — roughly 650 light-years — and is intrinsically very luminous, radiating about 56,000 times the Sun's energy. Its surface temperature of around 26,000 K makes it one of the hottest stars visible to the naked eye, but most of its radiation is in the ultraviolet.

Observing Tips

Easy to locate as the lower-left star of Orion's main quadrilateral, opposite Betelgeuse. Saiph appears blue-white but slightly fainter than Rigel in the opposite corner. It is visible from virtually all inhabited latitudes. Best observed from December through March when Orion dominates the evening sky. Compare Saiph's blue-white color with Betelgeuse's reddish orange for a striking contrast.

History

The name Saiph comes from the Arabic 'saif al-jabbar,' meaning 'the sword of the giant.' However, modern constellation figures place Saiph at Orion's knee or foot rather than near his sword. The star's position in Orion has made it a navigation reference point for thousands of years across many cultures.

Fun Facts

Saiph appears similar in brightness to Rigel, but the two could hardly be more different intrinsically. Saiph is hotter than Rigel but appears fainter because it radiates more of its energy as invisible ultraviolet light. If our eyes could see UV, Saiph would be the brightest star in Orion.

Observe

1Physical Properties

Magnitude 2.06
Range 2.04 - 2.09
Variable Type ACYG
Spectral Type B0II bright giant
Star Color Blue (B-V -0.17)
Distance 646 ly

2Position & Identifiers

RA 05h 47m 45.4s
Dec -09° 40' 11.0"
Constellation Orion (Ori)
HR 2004
HIP 27366
HD 38771
SAO 132542
Bayer Kappa
Flamsteed 53 Ori

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 Nov – Jan (peak: Dec)

5Survey Image

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Explore

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Size Comparison

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Compare Stars

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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

Color excess E(B-V) = +0.07.
Ori OB1.
Deficient in ultraviolet relative to most early-type supergiants shortward of 2800A.
SAIPH.
Diam. 0.00044 - 0.00045".
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Light Travel Time Machine

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Relativistic Travel

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