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Alkaphrah — Double Star in Ursa Major

HIP 44471; Kappa Ursae Majoris; 12 Ursae Majoris

Magnitude 3.6m DoubleStar Ursa Major (UMa) Visible
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About Alkaphrah

Description

Alkaphrah, Kappa Ursae Majoris, is an A1 III giant about 360 light-years away, forming the southern half of the First Leap of the Gazelle with Talitha (Iota UMa). Alkaphrah is itself a close binary, with two nearly equal components about 0.05 arcseconds apart and an orbital period of roughly 36 years — too close for visual resolution in amateur scopes. Combined magnitude is 3.60.

Observing Tips

Alkaphrah and Talitha lie about 0.7 degrees apart west of the main Big Dipper, forming one of the sky's most graceful bright pairs. In binoculars they show distinct colors: Alkaphrah is pure white-blue, Talitha slightly yellower. The close binary within Alkaphrah is a spectroscopic target; visual observers see only one point of light. Circumpolar from mid-northern latitudes.

History

The name Alkaphrah comes from the Arabic "al-qafrah" (the springing), referring to the leap of the gazelle fleeing the bear's paws in pre-Islamic astronomy. The spectroscopic binary nature was identified through radial-velocity measurements in the early 20th century.

Fun Facts

Despite its Bayer designation of Kappa (the tenth letter), Alkaphrah is one of the brighter stars on the outskirts of Ursa Major and serves as a handy signpost for locating the more distant faint galaxies of Leo and Lynx that lie just to the south.

Observe

1Physical Properties

Magnitude 3.60
Spectral Type A1III giant
Star Color White (B-V 0.00)
Distance 357 ly

2Position & Identifiers

RA 09h 03m 37.5s
Dec +47° 09' 24.0"
Constellation Ursa Major (UMa)
HR 3594
HIP 44471
HD 77327
SAO 42661
Bayer Kappa
Flamsteed 12 UMa
Double Cat 7158

3How easy to spot?

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Equipment Bortle 3 Bortle 4 Bortle 5
Naked eye Easy Medium+ Medium+
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 Jan – Mar (peak: Feb)

5Multiple Star System

Separation 0.3″
Companion Mag 4.5
Position Angle 278°
Star Colors A: White B: Yellow-white
Discoverer A 1585
4.2 A0IV-V, 4.4 A0V, 70.1y, a = 0.27" or 64.29y, a = 0.26". Mag., colors for combined light.

Separation over time

Period: 8.2 y Eccentricity: 0.558 Now: 0.27", PA 283° -0.13" in 5 years
0.00" 0.08" 0.16" 0.24" 0.33" 2024 2026 2028 2030 0.27"

Apparent separation over time, computed from ORB6 orbital elements. Steep curves indicate fast-changing pairs — catch them while they're splittable.

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

Discover

15Stellar Notes

0.009".
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Light Travel Time Machine

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Relativistic Travel

Nearby in the Sky

Other targets within a few degrees — pan your scope a little and keep exploring.

Visibility scores assume a 150 mm Newton at Bortle 4.

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