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Menkalinan — Star in Auriga

Beta Aur

Magnitude 1.9m Star Auriga (Aur) Visible
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About Menkalinan

Description

Menkalinan is a white subgiant of spectral type A2IV at magnitude 1.90 in Auriga. Located about 82 light-years from Earth, it is an eclipsing binary system — two nearly identical A-type stars orbiting each other every 3.96 days, causing small dips in brightness as each passes in front of the other. Combined luminosity is about 95 times solar.

Observing Tips

Menkalinan is the second brightest star in Auriga after Capella, located about 7 degrees to the east-southeast. It helps define the pentagon shape of the Charioteer. Its white color contrasts with Capella's golden hue. Best observed November through April when Auriga is high in the winter sky.

History

The name Menkalinan comes from the Arabic 'mankib dhi'l-'inan,' meaning 'the shoulder of the rein-holder,' describing its position in the Charioteer figure. Its eclipsing binary nature was discovered spectroscopically in the early 20th century.

Fun Facts

Menkalinan's two nearly identical stars are so close together that they orbit each other in under 4 days. The eclipses cause brightness dips of only about 0.1 magnitude — too small to notice visually but easily measured with instruments.

Observe

1Physical Properties

Magnitude 1.90
Range 1.89 - 1.98
Period 4.0 days
Variable Type Eclipsing Binary (Algol-type)
Spectral Type A1V
Star Color White (B-V 0.03)
Distance 80 ly

2Position & Identifiers

RA 05h 59m 31.7s
Dec +44° 56' 51.0"
Constellation Auriga (Aur)
HR 2088
HIP 28360
HD 40183
SAO 40750
Bayer Beta
Flamsteed 34 Aur
Variable ID Bet Aur
Double Cat 4556

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 Nov – Jan (peak: Dec)

5Survey Image

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Explore

7

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

13

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

ADS 4556A, EA 1.89 - 1.98V, 1.93 - 2.02B, A2+A2, 3.9600421d, i 78.5d.
AB binary. C, 14.1v at 13".
ADS 4556A, 3.9600d, K 107.5k/s, V0 -17.1k/s, msin3i 2.20, asini 5.85. Masses 2.33, 2.25 solar. Rotational | velocities both components <30k/s. Second SB ever discovered, by Antonia Maury, 1889.
In Ursa cluster; Sirius group; UMa stream; UMa cluster.
Menkalinan; Menkalina.
Radius relative to Sun = 3.0.
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Light Travel Time Machine

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Relativistic Travel

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