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Algieba — Double Star in Leo

HIP 50583; Gamma1 Leonis; 41 Leonis

Observable Double Star Showpiece (77/100)

Sep: 4.8", Companion: mag 3.6

Magnitude 1.8–2.0m DoubleStar Leo Visible 1 Exoplanet
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About Algieba

Description

Algieba is one of the finest double stars in the sky at magnitude 2.61 in Leo. A small telescope reveals a stunning pair — a golden-orange giant (K1III, mag 2.3) and a slightly fainter yellow-green companion (G7III, mag 3.5) separated by about 4.5 arcseconds. Located about 126 light-years from Earth, the primary has a confirmed exoplanet.

Observing Tips

Algieba lies in the Sickle of Leo, the curved line of stars forming the Lion's head. In a telescope at 100x or more, it splits into a gorgeous warm-toned double — golden orange and yellowish green. It rivals Almach and Albireo as one of the most beautiful double stars. Best observed February through June.

History

The name Algieba comes from the Arabic 'al-jabhah,' meaning 'the forehead.' The double star nature was first observed in 1782 by William Herschel. In 2009, a giant exoplanet (Gamma Leo b) with about 8.8 Jupiter masses was discovered orbiting the primary.

Fun Facts

Algieba's color contrast — deep gold and pale green — makes it one of the most beautiful doubles in the northern sky. The 'green' star is likely an optical illusion enhanced by contrast with the orange primary, as truly green stars do not exist.

Observe

1Physical Properties

Magnitude 2.61
Range 1.98 - 2.02
Variable Type RS CVn (Chromospherically Active)
Spectral Type K1-IIIbFe-0.5
Star Color Orange (B-V 1.15)
Distance 148 ly

2Position & Identifiers

RA 10h 19m 58.3s
Dec +19° 50' 30.0"
Constellation Leo
HR 4057
HIP 50583
HD 89484
SAO 81298
Bayer Gamma1
Flamsteed 41 Leo
Double Cat 7724

3How easy to split?

Primary 2.6 mag Companion 3.6 mag Separation 4.8″
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Telescope Bortle 3 Bortle 4 Bortle 5
80mm refr. Easy Easy Easy
150mm Newt. Easy Easy Easy
C8 203mm 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 Quadruple C,D: optical

Components 4 (quadruple)
Component IDs AB
Separation 4.8″
Companion Mag 3.6
Companion Sp gG7
Position Angle 127°
Star Colors A: Orange B: Orange
Discoverer STF1424
AB 2.22 K0IIIP, 3.47 G7III, 618.56y, a = 2.505". B is HR 4058. Colors for combined light. Mag. for blend, 1.90V. | Component C is the flare star AD Leo (8.07-11.00B) at 5', optical.

Separation over time

Period: 554.0 y Eccentricity: 0.930 Now: 4.7", PA 127° + 0.01" in 5 years
0.00" 1.4" 2.8" 4.1" 5.5" 2025 2030 2035 2040 2045 4.7"

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

Eyepiece View

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80x Dawes: 1.9″ TFOV: 0.6°
Realistic = true angular size
N E 127°

A: 2.6 · B: 3.6 · Sep: 4.8″ · PA: 127° · N up, E right

Resolved · Rayleigh: 2.3″ · Dawes: 1.9″ · Eff: 2.3″

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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Exoplanets 1 known planet

View in 3D
View this system in the 3D Orrery
Interactive Keplerian orbits, procedural planet textures, habitable zone.
Planet Radius Mass Period Distance
gam1 Leo b 12.50R⊕ 8.78M♃ 1.2yr 130ly

Habitable Zone

Size & Mass Comparison

About exoplanets — how we find them and which host stars you can observe

Discover

16Stellar Notes

Originally confused with eclipsing star Y Leo when var. suspect number 6777 was assigned in 1965. Now HR 4057 is again | suspected of variability, 1.84 - 2.03V for combined HR 4057/8. Uncertain which component is the variable.
Gamma Leo group.
0.013".
ALGIEBA; Algeiba; Al Gieba.
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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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