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Suhail Hadar — Estrella en Popa

HIP 39429; Zeta Puppis

Magnitud 2.2m Star Popa (Pup) Visible
Mapa Estelar
+ Lista + Plan

Acerca de Suhail Hadar

Descripción

Naos (also known as Suhail Hadar) is one of the hottest and most luminous stars visible to the simple vista. At tipo espectral O5Iaf and magnitude 2.25, it is a supergigante azul with a temperatura superficial of about 42,000 K and a luminosity roughly 800,000 times that of el Sol. Located aproximadamente 1,080 años luz away, Naos has a powerful viento estelar that ejects mass at a rate millions of times greater than el Sol's solar wind.

Consejos de Observación

Located in the southeastern part of Puppis, Naos is a striking blue-white star best viewed from the hemisferio sur or from low latitudes boreales. It sits in a rich part of the Vía Láctea with many background stars. Prismaticos reveal its vivid blue-white color against the star-rich backdrop. Mejor observación from January through April. From northern mid-latitudes it is low on the southern horizon.

Historia

The name Naos comes from the Greek 'naos,' meaning 'ship,' referring to the constellation Puppis (the stern of the mythological ship Argo). The alternate name Suhail Hadar is Arabic in origin. Zeta Pup was one of the first stars whose extreme temperature was determined spectroscopically, revealing it as an O-type supergiant — among the most massive and energetic stars known.

Datos Curiosos

Naos is a stellar powerhouse — if placed where el Sol is, it would appear 16,700 times brighter and would completely sterilize all planets in the sistema solar with its intense ultraviolet radiation. It is also a runaway star, hurtling through space at an unusually high velocity, likely ejected from a sistema binario when its companion exploded as a supernova.

Observar

1Propiedades Físicas

Magnitud 2.25
Rango 2.24 - 2.26
Período 42.7 horas
Tipo variable ROT:
Tipo Espectral O6/7III
Color de la Estrella Azul (B-V -0.26)
Distancia 1,082 ly

2Posición e Identificadores

RA 08h 03m 35.1s
Dec -40° 00' 12.0"
Constelación Popa (Pup)
HR 3165
HIP 39429
HD 66811
SAO 198752
Bayer Zeta

3Dificultad de observación

Iniciar sesión y configura tu equipo y ubicación predeterminada para ver una fila personalizada.
Equipo Bortle 3 Bortle 4 Bortle 5
Simple vista Fácil Fácil Fácil
Buscador 50mm Fácil Fácil Fácil
150mm telesc. Fácil Fácil Fácil
Fácil Medio Difícil Muy difícil Imposible

Bortle 3 = rural · 4 = suburbano · 5 = urbano

4Visibilidad

Establece una ubicación en Ajustes de Usuario para ver datos de visibilidad.

Mejor temporada Dec – Feb (peak: Jan)

5Imagen de Rastreo

Cargando imagen de rastreo…

Explorar

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Comparación de tamaño

Consultando VizieR para datos estelares…
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Comparar estrellas

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Clasificación espectral

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Diagrama de Hertzsprung-Russell

Cargando diagrama HR…
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Ciclo de vida estelar

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Espectro de cuerpo negro

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Espectro de absorción estelar

Espectro de absorción simulado basado en el tipo espectral. Pase el ratón sobre las líneas para identificar los elementos.

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Fusión Estelar

Descubrir

15Notas Estelares

Change in H alpha emission profile between 1974 and 1976 interpreted as change in rate of mass loss.
Color excess E(B-V) = +0.04.
In cluster CR 173; in HII region.
Also classified O4f, O4ef and O4I9n)f.
Naos; Suhail Hadar.
Diam. = 0.00041 - 0.00042".
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Máquina del tiempo de la luz

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Viaje Relativista

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