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Mu Velorum — Double Star in Vela

Observable Double Star Good (51/100)

Sep: 2.3", Companion: mag 5.7

Magnitude 2.7m DoubleStar Vela (Vel) Visible
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About Mu Vel

Description

Mu Velorum is a binary star system at magnitude 2.69 in Vela, consisting of a yellow giant (G5III) and a fainter yellow companion (G2V). Located about 117 light-years from Earth, the primary has a luminosity of roughly 107 times solar. The two components can be resolved in a small telescope.

Observing Tips

Mu Vel lies in the central part of Vela, separated from the other bright Vela stars. A small telescope resolves the pair at about 2.6 arcseconds separation. The color similarity of the two components (both yellow) makes this a subtle but pleasing double. Visible from the southern hemisphere. Best observed February through May.

History

Mu Velorum has no traditional proper name. As part of the former Argo Navis constellation, it was designated by Lacaille during his southern sky survey from the Cape of Good Hope in the 1750s.

Fun Facts

Mu Vel's secondary component is a G2V star — the same spectral type as our Sun. Seeing it next to the evolved giant primary gives a visual impression of what the Sun's companion might look like if the Sun had a giant star nearby.

Observe

1Physical Properties

Magnitude 2.69
Spectral Type G6III giant
Star Color Orange (B-V 0.90)
Distance 117 ly

2Position & Identifiers

RA 10h 46m 46.2s
Dec -49° 25' 12.0"
Constellation Vela (Vel)
HR 4216
HIP 52727
HD 93497
SAO 222321
Bayer Mu

3How easy to split?

Primary 2.7 mag Companion 5.7 mag Separation 2.3″
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Telescope Bortle 3 Bortle 4 Bortle 5
80mm refr. Hard Hard Hard
150mm Newt. Medium Medium Medium
C8 203mm Medium+ Medium+ Medium+
Easy Medium Hard Very hard Impossible

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

4Visibility

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Best season Jan – Mar (peak: Feb)

5Multiple Star System

Separation 2.3″
Companion Mag 5.7
Companion Sp G2V
Position Angle 59°
Star Colors A: Orange B: Yellow
Discoverer R 155
2.7 G5III, 6.4 G2V, 116.24y, a = 1.437". Secondary also classified F8:V:.

Separation over time

Period: 142.9 y Eccentricity: 0.940 Now: 2.3", PA 59° -0.01" in 5 years
0.00" 0.67" 1.3" 2.0" 2.7" 2025 2030 2035 2040 2045 2.3"

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 59°

A: 2.7 · B: 5.7 · Sep: 2.3″ · PA: 59° · 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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15Stellar Notes

Sirius group?
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Light Travel Time Machine

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Relativistic Travel

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