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Iota Ceti — Double Star in Cetus

DoubleStar Cetus (Cet) Visible
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Observe

1Physical Properties

Magnitude 3.56
Range 3.54 - 3.58
Variable Type Variable (Unclassified)
Spectral Type K1 II + (K)
Star Color Red (B-V 1.22)
Distance 274 ly

2Position & Identifiers

RA 00h 19m 25.7s
Dec -08° 49' 26.0"
Constellation Cetus (Cet)
HR 74
HIP 1562
HD 1522
Bayer Iota
Flamsteed 8 Cet

3How easy to split?

Primary 3.6 mag Companion 10.4 mag Separation 106.4″
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Telescope Bortle 3 Bortle 4 Bortle 5
80mm refr. Medium Hard+ Hard+
150mm Newt. Easy Medium+ Medium+
C8 203mm Easy Easy Medium+
Easy Medium Hard Very hard Impossible

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

4Visibility

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Best season Aug – Oct (peak: Sep)

5Multiple Star System Triple C: optical

Components 3 (triple)
Component IDs AC
Separation 106.4″
Companion Mag 10.4
Position Angle 191°
Star Colors A: Red
Discoverer HJ 1953
Component B, 12.87v at 63", optical.

Separation over time

Measured 1892 → 2014 (122 y)
Separation drift 109.8" → 106.4" (-3.40")
Rate -0.0279" / y
PA drift 198° → 191° (-7°, -0.057°/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 191°

A: 3.6 · B: 10.4 · Sep: 106.4″ · PA: 191° · N up, E left

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

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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.

14

Stellar Fusion

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15Stellar Notes

3.46 - 3.56V.
Deneb Kaitos Shemali; Deneb Kaitos Al Shamaliyy.
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Light Travel Time Machine

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Relativistic Travel

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