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Alnilam

HIP 26311; Epsilon Ori; 46 Ori

HIP 26311; Epsilon Ori; 46 Ori DoubleStar Ori Visível Nível 3 Medium telescope (6-8") - Requires steady seeing
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Propriedades Físicas

Magnitude 1.70
Tipo Espectral B0Ib
Cor da Estrela Azul (B-V -0.19)
Temperatura 27526 K
Raio 32.4 R☉
Distância 1341.2 ly

Posição e Identificadores

RA 05h 36m 12.8s
Dec -01° 12' 07.0"
Constelação Ori
HR 1903
HIP 26311
Bayer Epsilon
Flamsteed 46 Ori
Variable ID f

Visibilidade

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Sistema Estelar Múltiplo

Separação 179.5″
Mag da Companheira 11.3
Ângulo de Posição 58°
Cores das Estrelas A: Azul
Descobridor BUP 81

Vista pela Ocular

32x Dawes: 1.9″ TFOV: 1.6°
Realista = tamanho angular verdadeiro
N E 58° A (1.7) B (11.3)

Sep: 179.5″ · PA: 58° · 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

Alpha Cyg 1.64 - 1.74V.
In both infrared survey and UV CELESCOPE. Color excess E(B-V) = +0.08.
Ori OB1b2; Orion belt; cluster NGC 1980; nebulosity.
Nitrogen deficient. Interstellar Lyman alpha absorption observed by AEROBEE rocket. Walborn declares "no e", but | Merrill found H alpha emission.
UV AEROBEE spectra indicate mass ejection at velocity up to 1800k/s.
ALNILAM; Alnihan; Alnitam.
Diam. = 0.00067 - 0.00069".

Imagem de Levantamento

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Sobre Alnilam

Descrição

Alnilam is a blue supergiant of spectral type B0Ia, the middle and brightest star of Orion's Belt at magnitude 1.70. Located about 2,000 light-years from Earth, it is one of the most distant bright stars visible to the naked eye. Alnilam is extraordinarily luminous — roughly 275,000 times the luminosity of the Sun — and has about 40 times the Sun's mass. It is losing mass rapidly through powerful stellar winds.

Dicas de Observação

Alnilam is the middle star of Orion's famous Belt, flanked by Alnitak to the east and Mintaka to the west. The three Belt stars are one of the most recognizable patterns in the night sky. Through binoculars, the surrounding region is rich with nebulosity — the emission nebula NGC 1990 surrounds Alnilam itself. The Belt points downward to Sirius and upward to Aldebaran, making it an excellent starting point for star-hopping. Best observed from November through March.

História

The name Alnilam comes from the Arabic 'al-Nilam' meaning 'string of pearls,' referring to the line of Belt stars. Orion's Belt is one of the most universally recognized star patterns across human cultures — it has been identified with three kings, three sisters, a celestial bridge, and many other mythological figures worldwide. The ancient Egyptians aligned the three Great Pyramids of Giza to mirror the Belt stars.

Curiosidades

At roughly 275,000 solar luminosities, Alnilam is one of the most luminous stars known in the Milky Way. Its powerful stellar wind blows at over 2,000 km/s, and it is losing mass at a rate millions of times greater than the Sun's solar wind. The alignment of the three Pyramids of Giza with Orion's Belt (the Orion Correlation Theory) is one of the most popular — and debated — claims in archaeoastronomy.