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Murzim — Double Star in Canis Major

Beta CMa

Magnitude 2.0m DoubleStar Canis Major (CMa) Visible
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About Murzim

Description

Murzim (also spelled Mirzam) is a blue giant of spectral type B1II-III at magnitude 1.98 in Canis Major. Located about 500 light-years from Earth, it has a luminosity of roughly 26,600 times solar. Murzim is a Beta Cephei variable, pulsating with a period of about 6 hours, though the brightness change is very small.

Observing Tips

Murzim lies about 5 degrees west of Sirius, making it easy to find. It appears as a bright blue-white star that 'heralds' the rising of Sirius. Look for it as the first bright star to rise before Sirius clears the horizon. Best observed December through March.

History

The name Murzim (or Mirzam) comes from the Arabic 'al-murzim,' meaning 'the announcer,' because it rises shortly before Sirius and thus 'announces' the arrival of the brightest star. This herald-role gave it significance in cultures that closely watched for Sirius's appearance.

Fun Facts

Murzim is intrinsically over 1,000 times more luminous than Sirius, yet appears fainter because it is nearly 60 times farther away. Its role as Sirius's announcer was important in ancient Egypt, where the heliacal rising of Sirius marked the start of the flood season.

Observe

1Physical Properties

Magnitude 1.98
Range 1.97 - 2.00
Period 6.0 hours
Variable Type Beta Cephei (Pulsating)
Spectral Type B1III giant
Star Color Blue (B-V -0.23)
Distance 492 ly

2Position & Identifiers

RA 06h 22m 42.0s
Dec -17° 57' 21.0"
Constellation Canis Major (CMa)
HR 2294
HIP 30324
HD 44743
SAO 151428
Bayer Beta
Flamsteed 2 CMa
Variable ID Bet CMa

3How easy to split?

Primary 2.0 mag Companion 10.5 mag Separation 186.1″
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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 Nov – Jan (peak: Dec)

5Light Curve

6Multiple Star System

Separation 186.1″
Companion Mag 10.5
Position Angle 340°
Star Colors A: Blue
Discoverer BUP 88

Separation over time

Measured 1879 → 2010 (131 y)
Separation drift 185.0" → 186.1" (+1.10")
Rate +0.0084" / y
PA drift 339° → 340° (+1°, +0.008°/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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32x Dawes: 1.9″ TFOV: 1.6°
Realistic = true angular size
N E 340°

A: 2.0 · B: 10.5 · Sep: 186.1″ · PA: 340° · 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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16Stellar Notes

Beta C 1.93 - 2.00V. Prototype star. Multi-periodic: 0.25002246, 0.2513003, 49.17 and 0.23904d, others reported. Beat | periods 49.198, 5.442 and 4.900d. Sp. also var. over 0.25d.
Color excess E(B-V) = +0.01.
Lyman alpha and Lyman beta observed from COPERNICUS.
0.25002246 and 49d.
Murzim; Mirzam; Mirza.
Diam. = 0.00050 - 0.00052".
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Light Travel Time Machine

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Relativistic Travel

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