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Chi Centauri — Double Star in Centaurus

Observable Double Star Good (53/100)

Sep: 85.2", Companion: mag 8.5

Magnitude 4.4m DoubleStar Centaurus (Cen) Visible
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1Physical Properties

Magnitude 4.36
Spectral Type B2V
Star Color Blue (B-V -0.19)

2Position & Identifiers

RA 14h 06m 02.8s
Dec -41° 10' 47.0"
Constellation Centaurus (Cen)
HR 5285
HIP 68862
HD 122980
SAO 224673
Bayer Chi
Variable ID Chi Cen

3How easy to split?

Primary 4.4 mag Companion 8.5 mag Separation 85.2″
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Telescope Bortle 3 Bortle 4 Bortle 5
80mm refr. Easy Easy Medium+
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 Mar – May (peak: Apr)

5Multiple Star System

Separation 85.2″
Companion Mag 8.5
Companion Sp K3Ve
Position Angle 78°
Star Colors A: Blue B: Orange
Discoverer WFC 145

Separation over time

Measured 1826 → 2016 (190 y)
Separation drift 77.6" → 85.2" (+7.60")
Rate +0.0400" / y
PA drift 77° → 78° (+1°, +0.005°/y)

Apparent motion is significant on a human timescale — worth revisiting in a decade.

Measured from the WDS observational archive. No orbital solution has been derived — most likely the period is too long to fit an orbit to the available measurement arc.

Eyepiece View

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80x Dawes: 1.9″ TFOV: 0.6°
Realistic = true angular size
N E 78°

A: 4.4 · B: 8.5 · Sep: 85.2″ · PA: 78° · N up, E right

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

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7

Size Comparison

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8

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9

Spectral Classification

10

Hertzsprung-Russell Diagram

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11

Stellar Lifecycle

12

Blackbody Spectrum

13

Stellar Absorption Spectrum

Simulated absorption spectrum based on spectral type. Hover over lines to identify elements.

14

Stellar Fusion

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15Stellar Notes

Amp. 0.020B, 0.035d.
Sco-Cen cluster; upper Cen group of Sco-Cen assoc.; member of Pleiades group.
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