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Capella

HIP 24608; Alpha Aur; 13 Aur

HIP 24608; Alpha Aur; 13 Aur DoubleStar Aur Visível Nível 3 Medium telescope (6-8") - Requires steady seeing
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Propriedades Físicas

Magnitude 0.08
Tipo Espectral G1III + K0III
Cor da Estrela Laranja (B-V 0.80)
Temperatura 4891 K
Raio 11.9 R☉
Distância 43.3 ly

Posição e Identificadores

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

Visibilidade

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Sistema Estelar Múltiplo

Componentes 10
IDs dos Componentes AP
Separação 91.5″
Mag da Companheira 17.1
Ângulo de Posição
Cores das Estrelas A: Laranja
Descobridor BAR 25

Vista pela Ocular

80x Dawes: 1.9″ TFOV: 0.6°
Realista = tamanho angular verdadeiro
N E A (0.1) B (17.1)

Sep: 91.5″ · PA: 6° · N cima, L esquerda

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

Comparação de Tamanho

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Classificação Espectral

Diagrama Hertzsprung-Russell

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Espectro de corpo negro

Espectro de absorção estelar

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Notas Estelares

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".

Imagem de Levantamento

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Sobre Capella

Descrição

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.

Dicas de Observação

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.

História

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.

Curiosidades

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.