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HIP 66223 — Double Star in Canes Venatici

Magnitude 6.4m DoubleStar Canes Venatici (CVn) Visible
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Observe

1Physical Properties

Magnitude 6.37
Spectral Type F0IV subgiant
Star Color Yellow-white (B-V 0.21)

2Position & Identifiers

RA 13h 34m 21.8s
Dec +38° 47' 21.0"
HR 5108
HIP 66223
HD 118156
SAO 63616
Double Cat 8956

3How easy to split?

Primary 6.4 mag Companion 10.5 mag Separation 28.5″
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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 Mar – May (peak: Apr)

5Multiple Star System B: optical

Separation 28.5″
Companion Mag 10.5
Position Angle
Star Colors A: Yellow-white
Discoverer HJ 1234
Optical.

Separation over time

Measured 1896 → 2015 (119 y)
Separation drift 33.4" → 28.5" (-4.90")
Rate -0.0412" / y
PA drift 23° → 5° (-18°, -0.151°/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

A: 6.4 · B: 10.5 · Sep: 28.5″ · PA: 5° · 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

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