Menu

Shaula

HIP 85927; Lambda Sco; 35 Sco

HIP 85927; Lambda Sco; 35 Sco DoubleStar Sco Visível Nível 3 Medium telescope (6-8") - Requires steady seeing
Mapa Estelar Adicionar à Lista Adicionar ao Plano
Voltar ao Catálogo

Propriedades Físicas

Magnitude 1.63
Tipo de Variável Beta Cephei (Pulsating)
Tipo Espectral B1.5 IV + B
Cor da Estrela Azul (B-V -0.22)
Distância 570.0 ly

Posição e Identificadores

RA 17h 33m 36.5s
Dec -37° 06' 14.0"
Constelação Sco
HR 6527
HIP 85927
Bayer Lambda
Flamsteed 35 Sco
Variable ID Lam Sco

Visibilidade

Defina um local nas Configurações do Usuário para ver dados de visibilidade.

Sistema Estelar Múltiplo

Componentes 3
IDs dos Componentes AC
Separação 42.4″
Mag da Companheira 14.9
Espectro da Companheira B
Ângulo de Posição 106°
Cores das Estrelas A: Azul B: Azul
Descobridor SEE 334

Vista pela Ocular

80x Dawes: 1.9″ TFOV: 0.6°
Realista = tamanho angular verdadeiro
N E 106° A (1.6) B (14.9)

Sep: 42.4″ · PA: 106° · N cima, L esquerda

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

Comparação de Tamanho

Consultando VizieR para dados estelares…

Ciclo de vida estelar

Classificação Espectral

Diagrama Hertzsprung-Russell

Carregando diagrama HR…

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

Beta C 1.59 - 1.65V, 0.2137015d, secondary 0.1068518d, beat period 10.1605d. Also possible 0.04V eclipse. X-ray | flare observed in vicinity Lambda Sco on 1 June 1975.
5.6d. Interferometer measures indicate multiple star.
Color excess E(B-V) = +0.03.
Sco-Cen assoc.
Lyman alpha and Lyman beta observed from COPERNICUS.
SHAULA.

Imagem de Levantamento

Carregando imagem de levantamento…

Sobre Shaula

Descrição

Shaula (Lambda Scorpii) is a blue subgiant of spectral type B2IV, located about 570 light-years from Earth. At magnitude 1.63, it is the second brightest star in Scorpius (after Antares) and marks the tip of the Scorpion's tail, where the stinger would be. Shaula is actually a triple star system with a combined luminosity of about 36,000 times the Sun's. The primary is a Beta Cephei variable, pulsating with a period of about 4.7 hours.

Dicas de Observação

Shaula forms a close pair with Lesath (Upsilon Scorpii, magnitude 2.7) — together they are sometimes called the 'Cat's Eyes' at the tip of the Scorpion's tail. This close pair is a pretty sight in binoculars. The open clusters M6 (Butterfly Cluster) and M7 (Ptolemy's Cluster) lie just a few degrees to the north, making this region rich territory for binocular sweeping. Shaula is best observed from May through August from locations with a good southern horizon.

História

The name Shaula comes from the Arabic 'al-Shawla' meaning 'the raised tail,' describing its position at the tip of the scorpion's tail. The Shaula-Lesath pair was noted by many ancient cultures. In Polynesian navigation, these stars served as important waypoints for oceanic voyaging.

Curiosidades

Shaula's close visual pairing with Lesath is a line-of-sight coincidence — the two stars are at very different distances (Lesath is about 580 light-years away, nearly the same as Shaula, but they are unrelated gravitationally). The pair's proximity earned them the nickname 'Cat's Eyes' from Australian observers.