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Aldebaran

HIP 21421; Alpha Tau; 87 Tau

HIP 21421; Alpha Tau; 87 Tau DoubleStar Tau Visível Nível 3 Medium telescope (6-8") - Requires steady seeing
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Propriedades Físicas

Magnitude 0.85
Tipo de Variável Slow Irregular Variable
Tipo Espectral K5III
Cor da Estrela Vermelho (B-V 1.54)
Temperatura 3881 K
Raio 44.3 R☉
Distância 64.7 ly

Posição e Identificadores

RA 04h 35m 55.2s
Dec +16° 30' 33.0"
Constelação Tau
HR 1457
HIP 21421
Bayer Alpha
Flamsteed 87 Tau
Variable ID Alp Tau
Double Cat 3321

Visibilidade

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Sistema Estelar Múltiplo

Componentes 6
IDs dos Componentes AC
Separação 31.4″
Mag da Companheira 13.6
Espectro da Companheira M2
Ângulo de Posição 115°
Cores das Estrelas A: Vermelho B: Vermelho
Descobridor BU 550

Vista pela Ocular

80x Dawes: 1.9″ TFOV: 0.6°
Realista = tamanho angular verdadeiro
N E 115° A (0.8) B (13.6)

Sep: 31.4″ · PA: 115° · N cima, L esquerda

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

Comparação de Tamanho

Ciclo de vida estelar

Classificação Espectral

Diagrama Hertzsprung-Russell

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Espectro de corpo negro

Espectro de absorção estelar

Espectro de absorção simulado com base no tipo espectral. Passe o mouse sobre as linhas para identificar os elementos.

Notas Estelares

Lb 0.75 - 0.95V. Var. H and K emission.
AB binary. B is 13.5v, dM2 at 31". CD, 122" from A is 11.2, 13.6v sep. 2" also binary but independent of AB.
Hyades group.
IR emission envelope diam. 10". MgII emissions indicate a cooler shell surrounding the supergiant.
0.048".
ALDEBARAN; Cor Tauri; Parilicium.
Diam. Two determinations, 0.022" and 0.0237".

Imagem de Levantamento

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Sobre Aldebaran

Descrição

Aldebaran is an orange giant star of spectral type K5III, the brightest star in the constellation Taurus at magnitude 0.85. It is located about 65 light-years from Earth and is roughly 44 times the diameter of the Sun and 425 times more luminous. Aldebaran appears to be part of the Hyades star cluster but is actually a foreground star, less than half the distance to the cluster. It is a slightly irregular variable star with small amplitude variations.

Dicas de Observação

Aldebaran is easy to find by extending the line of Orion's Belt to the upper right. Its deep orange color is immediately apparent and makes a fine contrast with the blue Pleiades cluster about 12 degrees to its northwest. Through binoculars, the surrounding Hyades cluster provides a rich star field with Aldebaran as the jewel at its center. The Moon regularly occults Aldebaran (in certain years), offering dramatic disappearance and reappearance events visible through small telescopes. Best observed from November through March.

História

The name Aldebaran comes from the Arabic 'al-Dabaran' meaning 'the follower,' because it appears to follow the Pleiades across the sky. It was one of the four Royal Stars of ancient Persia (along with Regulus, Antares, and Fomalhaut), marking the vernal equinox around 3000 BC. Ptolemy listed it in the Almagest as one of the brightest stars in the sky.

Curiosidades

In 1997, a planet was tentatively detected orbiting Aldebaran — Aldebaran b, a gas giant about 6 times the mass of Jupiter with a 629-day orbit — though the claim has been debated. Aldebaran was the target of the Pioneer 10 spacecraft; if the probe were still headed that way, it would reach the star's vicinity in about 2 million years.