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Iota Pictoris — Double Star in Pictor

HIP 22531; Iota Pictoris

Observable Double Star Excellent (64/100)

Sep: 12.3", Companion: mag 6.2

Magnitude 5.6m DoubleStar Pictor (Pic) Visible
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Observe

1Physical Properties

Magnitude 5.61
Spectral Type F0IV subgiant
Star Color Yellow-white (B-V 0.33)

2Position & Identifiers

RA 04h 50m 55.2s
Dec -53° 27' 41.0"
Constellation Pictor (Pic)
HR 1563
HIP 22531
HD 31203
SAO 233709
Bayer Iota

3How easy to split?

Primary 5.6 mag Companion 6.2 mag Separation 12.3″
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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 Oct – Dec (peak: Nov)

5Multiple Star System

Separation 12.3″
Companion Mag 6.2
Companion Sp F4V
Position Angle 58°
Star Colors A: Yellow-white B: Yellow-white
Discoverer DUN 18
CPM with HR 1564. B-V for combined light.

Separation over time

Measured 1826 → 2015 (189 y)
Separation drift 12.6" → 12.3" (-0.30")
Rate -0.0016" / y
PA drift 60° → 58° (-2°, -0.011°/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 58°

A: 5.6 · B: 6.2 · Sep: 12.3″ · PA: 58° · 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

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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

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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