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24 Canis Majoris — Star in Canis Major

Magnitude 3.0m Star Canis Major (CMa) Visible
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About 24 CMa

Description

24 Canis Majoris (also known as Omicron2 CMa) is a blue supergiant of spectral type B3Iab at magnitude 3.02 in Canis Major. Located roughly 2,800 light-years from Earth, it is one of the most distant naked-eye stars and is intrinsically very luminous — roughly 70,000 times the Sun's luminosity. It is a massive, hot star in an advanced stage of evolution.

Observing Tips

24 CMa lies in the body of Canis Major, southeast of Sirius. It is a blue-white star surrounded by the rich star fields of the winter Milky Way. Best observed from January through March when Canis Major is well-placed in the evening sky. Despite its faintness compared to nearby Sirius, it is easily visible to the naked eye.

History

24 CMa is identified by its Flamsteed number rather than a Bayer designation, as it was not among the brightest stars assigned Greek letters by Johann Bayer. It has no traditional proper name. Its extreme luminosity and distance were not appreciated until modern spectroscopic classification revealed its supergiant nature.

Fun Facts

24 CMa is a supergiant that is inherently far more luminous than Sirius, the brightest star in the sky — if placed at Sirius's distance of 8.6 light-years, it would shine as bright as the quarter Moon. Its great distance is the only reason it appears as a modest 3rd-magnitude star.

Observe

1Physical Properties

Magnitude 3.02
Range 2.99 - 3.08
Period 24.4 days
Variable Type ACYG
Spectral Type B4Ia supergiant
Star Color Blue-white (B-V -0.08)
Distance 2,764 ly

2Position & Identifiers

RA 07h 03m 01.5s
Dec -23° 49' 60.0"
Constellation Canis Major (CMa)
HR 2653
HIP 33977
HD 53138
SAO 172839
Flamsteed 24 CMa

3How easy to spot?

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Equipment Bortle 3 Bortle 4 Bortle 5
Naked eye Easy Easy Easy
50mm finder Easy Easy Easy
150mm scope 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)

5Survey Image

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Explore

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Size Comparison

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Compare Stars

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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

Discover

15Stellar Notes

H alpha profile changes in 30 min. or less.
Color excess E(B-V) = +0.03.
Probable member OB group near Omicron CMa; Collinder 121 (#29).
Balmer lines suggest mass loss 10E-08 solar/year.
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Light Travel Time Machine

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Relativistic Travel

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