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Gamma Centauri — Double Star in Centaurus

Magnitude 2.2m DoubleStar Centaurus (Cen) Visible
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About Gamma Cen

Description

Gamma Centauri is a binary star system of spectral type A1IV at magnitude 2.17 in Centaurus. It consists of two nearly identical A-type stars orbiting each other every 83 years. Located about 130 light-years from Earth, the combined luminosity is roughly 120 times solar.

Observing Tips

Gamma Cen lies in the body of Centaurus, between the brilliant Alpha/Beta pointer pair and the constellation's northern stars. It can be resolved as a double star in a moderate telescope, with the two components currently about 1 arcsecond apart. Only visible from the southern hemisphere. Best observed March through July.

History

Gamma Centauri has no widely used traditional name. The double star nature was discovered by James Dunlop in 1826. Centaurus is one of the oldest and largest constellations, representing the wise centaur Chiron of Greek mythology.

Fun Facts

Gamma Cen's two nearly identical stars make it a 'twin' double star system — both components are A1 subgiants of similar brightness, making the pair appear as two equally matched jewels when resolved in a telescope.

Observe

1Physical Properties

Magnitude 2.17
Spectral Type A1IV+ subgiant
Star Color Blue-white (B-V -0.01)
Distance 130 ly

2Position & Identifiers

RA 12h 41m 31.0s
Dec -48° 57' 35.0"
Constellation Centaurus (Cen)
HR 4819
HIP 61932
HD 110304
SAO 223603
Bayer Gamma

3How easy to split?

Primary 2.2 mag Companion 2.9 mag Separation 0.8″
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Telescope Bortle 3 Bortle 4 Bortle 5
80mm refr. V. hard V. hard V. hard
150mm Newt. Hard Hard Hard
C8 203mm Hard Hard Hard
Easy Medium Hard Very hard Impossible

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

To reach "Medium" at Bortle 3, you'd need at least a 270 mm reflector.

4Visibility

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Best season Feb – Apr (peak: Mar)

5Multiple Star System Triple

Components 3 (triple)
Component IDs AB
Separation 0.8″
Companion Mag 2.9
Companion Sp A2V
Position Angle 19°
Star Colors A: Blue-white B: White
Discoverer HJ 4539
AB 2.9 A0III, 2.9 A0III, 84.50y, a = 0.930". Combined mag., colors.

Separation over time

Period: 83.6 y Eccentricity: 0.793 Now: 0.85", PA 14° + 0.25" in 5 years
0.00" 0.43" 0.86" 1.3" 1.7" 2025 2030 2035 2040 2045 0.85"

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 19°

A: 2.2 · B: 2.9 · Sep: 0.8″ · PA: 19° · N up, E right

Unresolved · 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

12

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

Probably bluest member of Hyades group.
Hyades group.
0.024".
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Light Travel Time Machine

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Relativistic Travel

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