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Alpha Muscae — Star in Musca

Magnitude 2.7m Star Musca (Mus) Visible
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About Alpha Mus

Description

Alpha Muscae is a blue-white star of spectral type B2IV-V at magnitude 2.69, the brightest star in Musca (the Fly). Located about 315 light-years from Earth, it has a luminosity of roughly 4,520 times solar. It is a Beta Cephei variable with a pulsation period of about 2.2 hours.

Observing Tips

Alpha Mus lies just south of the Southern Cross in the small constellation Musca. It is a blue-white star in a rich region of the southern Milky Way. The Coal Sack dark nebula lies between Musca and Crux. Only visible from the southern hemisphere. Best observed March through June.

History

Musca was originally called 'Apis' (the Bee) by Petrus Plancius and was later renamed Musca (the Fly) by Lacaille. Alpha Muscae has no traditional proper name. The constellation is one of the smallest but most easily identified in the southern sky due to its proximity to the conspicuous Southern Cross.

Fun Facts

Musca is the only constellation named after an insect. Alpha Mus's rapid pulsation (2.2-hour period) makes it one of the shortest-period Beta Cephei variables among the bright stars.

Observe

1Physical Properties

Magnitude 2.69
Range 2.68 - 2.73
Period 2.2 hours
Variable Type Beta Cephei (Pulsating)
Spectral Type B2.5V
Star Color Blue (B-V -0.20)
Distance 315 ly

2Position & Identifiers

RA 12h 37m 11.0s
Dec -69° 08' 08.0"
Constellation Musca (Mus)
HR 4798
HIP 61585
HD 109668
SAO 251974
Bayer Alpha
Variable ID Alp Mus

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 Feb – Apr (peak: Mar)

5Survey Image

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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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15Stellar Notes

Beta C 2.68 - 2.73V, 2.17 - 2.24p, 0.0903d.
Companion B4V, optical.
Sco-Cen cluster; certain member of the Sco-Cen cluster; lower Cen group of Sco-Cen assoc.
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Light Travel Time Machine

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Relativistic Travel

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