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Beta Muscae — Double Star in Musca

Magnitude 3.0m DoubleStar Musca (Mus) Visible
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About Beta Mus

Description

Beta Muscae is a blue-white star of spectral type B2.5V at magnitude 3.05, the second brightest star in Musca. Located about 341 light-years from Earth, it is a close binary system with two blue stars orbiting every 194 years. Its combined luminosity is about 4,100 times solar.

Observing Tips

Beta Mus lies in the small constellation Musca just south of the Southern Cross. A moderate telescope can split the binary pair at their current separation. The dark Coal Sack nebula lies nearby. Only visible from the southern hemisphere. Best observed March through June.

History

Beta Muscae has no traditional proper name. Musca is one of the constellations created by Petrus Plancius from the observations of Dutch navigators and was originally known as 'Apis' (the Bee).

Fun Facts

Beta Mus is one of the more easily resolved bright binaries in the southern sky, with the two components slowly orbiting over nearly two centuries.

Observe

1Physical Properties

Magnitude 3.05
Spectral Type B2 V
Star Color Blue (B-V -0.18)
Distance 341 ly

2Position & Identifiers

RA 12h 46m 16.9s
Dec -68° 06' 29.0"
Constellation Musca (Mus)
HR 4844
HIP 62322
HD 110879
SAO 252019
Bayer Beta

3How easy to split?

Primary 3.1 mag Companion 4.0 mag Separation 0.9″
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Telescope Bortle 3 Bortle 4 Bortle 5
80mm refr. V. hard+ V. hard+ V. hard+
150mm Newt. Hard Hard Hard
C8 203mm Hard+ Hard+ Hard+
Easy Medium Hard Very hard Impossible

Bortle 3 = rural · 4 = outer suburbs · 5 = suburbs

To reach "Medium" at Bortle 3, you'd need at least a 250 mm reflector.

4Visibility

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Best season Feb – Apr (peak: Mar)

5Multiple Star System

Separation 0.9″
Companion Mag 4.0
Position Angle 58°
Star Colors A: Blue B: Yellow-white
Discoverer R 207
3.7 B2V, 4.0 B3V, 383.12y, a = 1.735". Combined mag., colors.

Separation over time

Period: 188.0 y Eccentricity: 0.790 Now: 0.91", PA 64° -0.05" in 5 years
0.00" 0.28" 0.55" 0.83" 1.1" 2025 2030 2035 2040 2045 0.91"

Apparent separation over time, computed from ORB6 orbital elements. Steep curves indicate fast-changing pairs — catch them while they're splittable.

Eyepiece View

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80x Dawes: 1.9″ TFOV: 0.6°
Realistic = true angular size
N E 58°

A: 3.0 · B: 4.0 · Sep: 0.9″ · PA: 58° · N up, E right

Unresolved · Rayleigh: 2.3″ · Dawes: 1.9″ · Eff: 2.3″

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

Sco-Cen assoc.
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Light Travel Time Machine

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Relativistic Travel

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