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Alniyat

HIP 80112; Sigma Sco; 20 Sco

HIP 80112; Sigma Sco; 20 Sco DoubleStar Sco Visible Niveau 3 Medium telescope (6-8") - Requires steady seeing
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Propriétés Physiques

Magnitude 2.89
Type variable Beta Cephei (Pulsating)
Type Spectral B1 III
Couleur de l'Étoile Blanc (B-V 0.13)
Distance 683.4 ly

Position et Identifiants

RA 16h 21m 11.3s
Dec -25° 35' 34.0"
Constellation Sco
HR 6084
HIP 80112
Bayer Sigma
Flamsteed 20 Sco
Variable ID Sig Sco
Double Cat 10009

Visibilité

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Système Stellaire Multiple

Composantes 4
IDs des Composantes O
Séparation 20.5″
Mag du Compagnon 8.4
Type Sp. du Compagnon B8V
Angle de Position 269°
Couleurs des Étoiles A: Blanc B: Bleu-blanc
Découvreur H 4 121

Vue à l'Oculaire

80x Dawes: 1.9″ TFOV: 0.6°
Réaliste = taille angulaire réelle
N E 269° A (2.9) B (8.4)

Sep: 20.5″ · PA: 269° · N en haut, E à gauche

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

Comparaison de taille

Interrogation de VizieR pour les données stellaires…

Cycle de vie stellaire

Classification spectrale

Diagramme de Hertzsprung-Russell

Chargement du diagramme HR…

Spectre du corps noir

Spectre d'absorption stellaire

Spectre d'absorption simulé basé sur le type spectral. Survolez les raies pour identifier les éléments.

Notes Stellaires

Beta C 2.94 - 3.06B. Multiple periods, 0.2468429, 0.239671, 8.2, and 33.1d. Surrounded by HII region. Primary | period varies in period of 23.2y with an amp. of 0.7 sec. Occultations indicate the variable has a 2.2 mag. fainter | companion at 0".49. The duplicity had been suspected from occultations as early as 1860. Orbital period probably over | 112 yrs. UV observations indicate temperature varies by 2510K and ratio max. to min. radius by 1.095.
B, 8.26V, +0.25(B-V), -0.23(U-B), B9.5V at 20", optical; vsini : 54k/s. The visual primary is triple: SB, 3.3, 5.3v, | sep. 0.0005" and 5.5v at 0.49", discovered by occultation.
ADS 10009A, 34.23d, K 34.0k/s, V0 +2.5k/s, asini 14.9.
Color excess E(B-V) = +0.40. Reddened star.
Sco OB2; Sco-Cen cluster; upper Sco region; HII region S9; in reflection nebula; assoc. Sco R1.
Stationary Ca lines. Although this star is an MK standard for class B1III, it is a variable, a multiple star, and is | situated in reflection nebulosity. Component A has also been classified as B2III and B2IV; component B as B9V, B9.5V, | and B8Vp. From scanner studies of composite spectra, Beavers (ApJS, 44, 489, 1980) finds ADS 10009A can be | resolved into O9.5 and B7 with a magnitude difference of 1.6V.
ADS 10009B, -6k/s.
Alniyat; Al Niyat. Name applies to pair with HR 6165.

Image de Relevé

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