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Capella

HIP 24608; Alpha Aur; 13 Aur

HIP 24608; Alpha Aur; 13 Aur DoubleStar Aur Visible Level 3 Medium telescope (6-8") - Requires steady seeing
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Physical Properties

Magnitude 0.08
Spectral Type G1III + K0III
Star Color Orange (B-V 0.80)
Temperature 4891 K
Radius 11.9 R☉
Distance 43.3 ly

Position & Identifiers

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

Visibility

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Multiple Star System

Components 10
Component IDs AP
Separation 91.5″
Companion Mag 17.1
Position Angle
Star Colors A: Orange
Discoverer BAR 25

Eyepiece View

80x Dawes: 1.9″ TFOV: 0.6°
Realistic = true angular size
N E A (0.1) B (17.1)

Sep: 91.5″ · PA: 6° · N up, E left

Resolved · Rayleigh: 2.3″ · Dawes: 1.9″ · Eff: 3.1″

Size Comparison

Stellar Lifecycle

Spectral Classification

Hertzsprung-Russell Diagram

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Blackbody Spectrum

Stellar Absorption Spectrum

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

Stellar 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".

Survey Image

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About Capella

Description

Capella is the sixth brightest star in the night sky at magnitude 0.08, located in the constellation Auriga about 43 light-years from Earth. It is actually a spectroscopic binary system consisting of two yellow giant stars: Capella Aa (spectral type G8III, about 79 solar luminosities) and Capella Ab (G1III, about 78 solar luminosities), orbiting each other every 104 days at a separation of about 0.74 AU. A distant pair of red dwarfs (Capella H and L) also belongs to the system.

Observing Tips

Capella is easily recognized as the brilliant yellowish star high in the northern sky during winter evenings. It forms a distinctive pentagon shape with the other bright stars of Auriga. The binary nature of Capella cannot be resolved visually — the two giant stars orbit too closely (0.05 arcseconds) — but their combined light makes a striking golden beacon. The nearby open clusters M36, M37, and M38 in Auriga make excellent binocular targets in the same region. Best observed from October through April. Capella is circumpolar from latitudes north of about 44°N.

History

The name Capella means 'little she-goat' in Latin, associated with the mythological goat Amalthea that suckled the infant Zeus. The Romans called it 'Capra.' It was listed in most ancient star catalogs, including Ptolemy's Almagest. The binary nature of Capella was discovered spectroscopically in 1899, and interferometric observations have since directly measured the orbit of the two giant components.

Fun Facts

Both giant stars of Capella are in a relatively brief evolutionary phase — they have exhausted the hydrogen in their cores and are now expanding and cooling. In a few million years, they will swell further into red giants. Capella is the closest first-magnitude star to the north celestial pole and one of the best-studied binary systems in the sky.