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Alfirk — Double Star in Cepheus

HIP 106032; Beta Cephei; 8 Cephei

Magnitude 3.2–3.3m DoubleStar Cepheus (Cep) Visible
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About Alfirk

Description

Alfirk is a blue giant of spectral type B1IV at magnitude 3.23 in Cepheus. Located about 690 light-years from Earth, it is the prototype of the Beta Cephei class of pulsating variable stars — massive hot stars that oscillate in brightness with periods of 3-7 hours. Alfirk's period is about 4.6 hours.

Observing Tips

Alfirk lies near the base of the house-shaped Cepheus, not far from Alderamin. It is a blue-white star circumpolar from mid-northern latitudes. Best observed August through December.

History

The name Alfirk comes from the Arabic 'al-firq,' meaning 'the flock.' As the prototype Beta Cephei variable, this star defines an important class of pulsating stars used to study the interiors of massive blue stars through asteroseismology.

Fun Facts

Beta Cephei variables are driven by an iron opacity mechanism — iron atoms deep in the stellar interior act as a valve, trapping heat and then releasing it, driving rhythmic pulsations. This mechanism was not understood until the 1990s.

Observe

1Physical Properties

Magnitude 3.23
Range 3.20 - 3.25
Period 4.6 hours
Variable Type Beta Cephei (Pulsating)
Spectral Type B1V
Star Color Blue (B-V -0.22)
Distance 682 ly

2Position & Identifiers

RA 21h 28m 39.6s
Dec +70° 33' 39.0"
Constellation Cepheus (Cep)
HR 8238
HIP 106032
HD 205021
SAO 10057
Bayer Beta
Flamsteed 8 Cep
Variable ID Bet Cep
Double Cat 15032

3How easy to split?

Primary 3.2 mag Companion 8.6 mag Separation 13.5″
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Telescope Bortle 3 Bortle 4 Bortle 5
80mm refr. Medium+ Medium+ 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 Jul – Sep (peak: Aug)

5Light Curve

6Multiple Star System Triple

Components 3 (triple)
Component IDs AB
Separation 13.5″
Companion Mag 8.6
Position Angle 248°
Star Colors A: Blue
Discoverer STF2806
ADS 15032AB, 50y. B, 7.84V, +0.18(B-V), +0.06(U-B), A2.5V, vsini 60:k/s. Third component discovered by speckle | interferometry, mag. diff about 4v. Sep. 0.025". Possible circumstellar material.

Separation over time

Measured 1779 → 2024 (245 y)
Separation drift 13.1" → 13.5" (+0.40")
Rate +0.0016" / y
PA drift 255° → 248° (-7°, -0.029°/y)

Essentially fixed on human timescales — the same view your grandchildren will see.

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 248°

A: 3.2 · B: 8.6 · Sep: 13.5″ · PA: 248° · N up, E right

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

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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

13

Blackbody Spectrum

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Stellar Absorption Spectrum

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

15

Stellar Fusion

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16Stellar Notes

ADS 15032A, Beta C 3.16 - 3.27V, 0.1904881d, modulation period 10.893d. SiIV and CIV vary. Satellite UV obs. | indicate temp. varies 1340d, max./min. radius 1.038.
ADS 15032A, 10.893d, K 3.1k/s, V0 -3.1k/s, asini 0.397. Resolved by speckle interferometry 1986.45, sep. 0.11".
Cep OB1.
0.004".
Alfirk; Alphirk.
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Light Travel Time Machine

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Relativistic Travel

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