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Spica

HIP 65474; Alpha Vir; 67 Vir

HIP 65474; Alpha Vir; 67 Vir DoubleStar Vir Visível Nível 3 Medium telescope (6-8") - Requires steady seeing
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Propriedades Físicas

Magnitude 0.98
Tipo de Variável Beta Cephei (Pulsating)
Tipo Espectral B1IV
Cor da Estrela Azul (B-V -0.23)
Temperatura 25412 K
Raio 7.4 R☉
Distância 249.9 ly

Posição e Identificadores

RA 13h 25m 11.6s
Dec -11° 09' 41.0"
Constelação Vir
HR 5056
HIP 65474
Bayer Alpha
Flamsteed 67 Vir
Variable ID Alp Vir

Visibilidade

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Sistema Estelar Múltiplo

Componentes 5
IDs dos Componentes O
Separação 151.9″
Mag da Companheira 12.0
Espectro da Companheira B2
Ângulo de Posição 33°
Cores das Estrelas A: Azul B: Azul
Descobridor BUP 150

Vista pela Ocular

80x Dawes: 1.9″ TFOV: 0.6°
Realista = tamanho angular verdadeiro
N E 33° A (1.0) B (12.0)

Sep: 151.9″ · PA: 33° · 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

Ell (Beta C) 0.97 - 1.04V, 4.01454d, and Beta C, 0.1737853d. Period changes.
Interferometer indicates visual component A is multiple system. Occultations yield three companions: 3.1v at 0.0025", | 4.5 at 0.05" and 7.5 at 0.5". Combined mag. and colors. Visual component B, 12.0v at 148".
4.0145d, K 120k/s, V0 0k/s, msin3i 7.16, asini 6.52. Rotation apsides 130 yrs. Rotational velocity 190k/s. | vsini secondary 102k/s.
Color excess E(B-V) = +0.03.
Also variously classified B2V+B2V, B1.5IV-V+B3V, B1V+B3V. Rocket observations show hydrogen lines Lyman alpha | through Zeta.
SPICA; Azimech; Spica Virginis; Alaraph, a name also given HR 4540, 4932.
Diam. = 0.00085 - 0.00087".

Imagem de Levantamento

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Sobre Spica

Descrição

Spica is the brightest star in Virgo and the 15th brightest in the night sky at magnitude 0.98. It is a blue giant of spectral type B1III-IV, located about 250 light-years from Earth. Spica is actually a close spectroscopic binary: two hot stars orbiting each other every 4.01 days at a separation of only about 0.12 AU. The primary is about 10 times the mass of the Sun and 12,000 times more luminous. The two stars are so close that they are tidally distorted into egg shapes.

Dicas de Observação

Spica is easy to find using the arc-to-Arcturus, spike-to-Spica mnemonic — follow the arc of the Big Dipper's handle through Arcturus and continue the curve to reach Spica. Its blue-white color contrasts sharply with the orange of nearby Arcturus. Spica is a useful reference star for the zodiac, as planets and the Moon frequently pass near it along the ecliptic. Best observed from March through July.

História

The name Spica comes from the Latin 'Spica Virginis' meaning 'ear of grain,' as it represents the sheaf of wheat held by the constellation Virgo. Hipparchus used observations of Spica around 130 BC to discover the precession of the equinoxes — one of the most important discoveries in ancient astronomy. Nicolaus Copernicus also observed Spica to refine his understanding of precession.

Curiosidades

The two stars of Spica are so close together that they are tidally distorted into ellipsoidal shapes, causing the system's brightness to vary by about 0.03 magnitudes as the elongated stars present different cross-sections to our line of sight. Spica is one of the 'pointer stars' for navigators and was critical to the discovery of precession over 2,000 years ago.