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HIP 34940 — Double Star in Canis Major

Magnitude 6.4m DoubleStar Canis Major (CMa) Visible
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1Physical Properties

Magnitude 6.36
Spectral Type B2IV+G5IV subgiant
Star Color Blue (B-V -0.21)

2Position & Identifiers

RA 07h 13m 48.3s
Dec -22° 54' 23.0"
Constellation Canis Major (CMa)
HR 2733
HIP 34940
HD 55856
SAO 173247
Double Cat 5912

3How easy to split?

Primary 6.4 mag Companion 9.1 mag Separation 19.3″
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Telescope Bortle 3 Bortle 4 Bortle 5
80mm refr. Easy 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 Dec – Feb (peak: Jan)

5Multiple Star System

Separation 19.3″
Companion Mag 9.1
Companion Sp G5IV
Position Angle 251°
Star Colors A: Blue B: Orange
Discoverer HJ 3938
Companion 9.07V, +0.77(B-V), +0.35(U-B), G1III or G5III, RV -3k/s, optical?

Separation over time

Measured 1837 → 2010 (173 y)
Separation drift 18.0" → 19.3" (+1.30")
Rate +0.0075" / y
PA drift 253° → 251° (-2°, -0.012°/y)

Slow change over generations — observable in lifetime comparisons.

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 251°

A: 6.4 · B: 9.1 · Sep: 19.3″ · PA: 251° · 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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