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Capella — Star in Auriga

HIP 24608; Alpha Aurigae; 13 Aurigae

Magnitude 0.1m Star Auriga (Aur) Visible
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About Capella

Description

Capella is the sixth brightest star in the sky and the brightest in Auriga. It is actually a spectroscopic binary system of two yellow giant stars (G8III + G0III) orbiting each other every 104 days, located about 43 light-years from Earth. The combined luminosity of the pair is roughly 80 times that of the Sun. A second, fainter pair of red dwarfs orbits the bright pair at a great distance, making Capella a quadruple star system.

Observing Tips

A brilliant golden-yellow star easily found high in the northern sky during winter evenings. It is circumpolar from most of Europe and northern North America, never setting below the horizon. At magnitude 0.08, it is unmistakable — look for the bright pentagon of Auriga with Capella as its most luminous vertex. Best in the evening sky from November through April. The close binary nature is not resolvable in any telescope.

History

The name Capella comes from Latin meaning 'little she-goat,' associated with the mythological goat Amalthea that suckled the infant Zeus. The ancient Romans called it 'the Goat Star.' Capella's binary nature was discovered spectroscopically in 1899 by William Campbell, and the orbital elements were refined over the following decades. The star has been important in many cultures — the Bedouins called it 'the Driver,' and in Hindu astronomy it was associated with the heart of Brahma.

Fun Facts

Capella is one of the few bright stars that is actually a close pair of giant stars of similar type — both have exhausted their core hydrogen and are evolving off the main sequence. Despite being so bright, Capella was one of the last bright stars to have its binary orbit fully determined because the pair is too close to resolve visually.

Observe

1Physical Properties

Magnitude 0.08
Range 0.05 - 0.10
Variable Type RS CVn (Chromospherically Active)
Spectral Type G1III + K0III giant
Star Color Orange (B-V 0.80)
Temperature 4891 K
Radius 11.9 R☉
Distance 43 ly

2Position & Identifiers

RA 05h 16m 41.4s
Dec +45° 59' 53.0"
Constellation Auriga (Aur)
HR 1708
HIP 24608
HD 34029
SAO 40186
Bayer Alpha
Flamsteed 13 Aur
Double Cat 3841

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

8

Compare Stars

9

Spectral Classification

10

Hertzsprung-Russell Diagram

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11

Stellar Lifecycle

12

Blackbody Spectrum

13

Stellar Absorption Spectrum

Simulated absorption spectrum based on spectral type. Hover over lines to identify elements.

14

Stellar Fusion

Discover

15Stellar Notes

Amp. 0.03V. Variable helium and X-ray emission.
AP 0.6 G5III, 1.1 G0III, sep. 0.04", 0.285y, a = 0.054", masses 2.67 and 2.55 solar. Combined mag., colors. Capella is | first star for which an orbit was determined from interferometer measures, by Anderson at Mt. Wilson in 1920. Speckle | sep. 0.040" 1981.24 and 1981.68; 0.055" 1982.16. CPM with component H, a close binary, 10.0 dM1, 13.7 dM5 sep. 2" at | 723" from A, probably physical with A. Other components all faint and distant from A.
104.0204d, K 26.1k/s, V0 +29.5k/s, asini 37.3.
Hyades group.
Chromospheric He 10830 double. Balloon-borne spectrometer revealed pronounced emission of MgII. Soft X-ray emission. | Lithium content of the F-type component is 15 times that of the G component. Also classified G6III+F9III.
0.058".
CAPELLA; Alhajoth.
Diam. component A = 0.0052", component B = 0.0040".
16

Light Travel Time Machine

17

Relativistic Travel

Nearby in the Sky

Other targets within a few degrees — pan your scope a little and keep exploring.

Visibility scores assume a 150 mm Newton at Bortle 4.

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