Menu

Capella — Estrella en Auriga

HIP 24608; Alpha Aurigae; 13 Aurigae

Magnitud 0.1m Star Auriga (Aur) Visible
Mapa Estelar
+ Lista + Plan

Acerca de Capella

Descripción

Capella is the sixth brightest star in the sky and the brightest en Auriga. It is actually a spectroscopic sistema binario of two gigante amarilla stars (G8III + G0III) orbiting each other every 104 days, located a unos 43 años luz de la Tierra. The combined luminosity of the pair is roughly 80 times that of el Sol. A second, fainter pair of enana rojas orbits the bright pair at a great distance, making Capella a quadruple star system.

Consejos de Observación

A brilliant golden-yellow star easily found high in the northern sky during invierno por la noche. It is circumpolar from most of Europe and northern North America, never setting below the horizon. At magnitude 0.08, it is unmistakable — look for the bright pentagon of Auriga with Capella as its most luminous vertex. Mejor en the cielo nocturno from November through April. The close binary nature is not resolvable in any telescopio.

Historia

The name Capella comes from Latin meaning 'little she-goat,' associated with the mythological goat Amalthea that suckled the infant Zeus. The ancient Romans called it 'the Goat Star.' Capella's binary nature was discovered spectroscopically in 1899 by William Campbell, and the orbital elements were refined over the following decades. The star has been important in many cultures — the Bedouins called it 'the Driver,' and in Hindu astronomy it was associated with the heart of Brahma.

Datos Curiosos

Capella is one of the few bright stars that is actually a close pair of giant stars of similar type — both have exhausted their core hydrogen and are evolving off the secuencia principal. Despite being so bright, Capella was one of the last bright stars to have its binary orbit fully determined because the pair is too close to resolve visually.

Observar

1Propiedades Físicas

Magnitud 0.08
Rango 0.05 - 0.10
Tipo variable RS CVn (Chromospherically Active)
Tipo Espectral G1III + K0III gigante
Color de la Estrella Naranja (B-V 0.80)
Temperatura 4891 K
Radio 11.9 R☉
Distancia 43 ly

2Posición e Identificadores

RA 05h 16m 41.4s
Dec +45° 59' 53.0"
Constelación Auriga (Aur)
HR 1708
HIP 24608
HD 34029
SAO 40186
Bayer Alpha
Flamsteed 13 Aur
Double Cat 3841

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 Nov – Jan (peak: Dec)

5Imagen de Rastreo

Cargando imagen de rastreo…

Explorar

7

Comparación de tamaño

8

Comparar estrellas

9

Clasificación espectral

10

Diagrama de Hertzsprung-Russell

Cargando diagrama HR…
11

Ciclo de vida estelar

12

Espectro de cuerpo negro

13

Espectro de absorción estelar

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

14

Fusión Estelar

Descubrir

15Notas Estelares

Amp. 0.03V. Variable helium and X-ray emission.
AP 0.6 G5III, 1.1 G0III, sep. 0.04", 0.285y, a = 0.054", masses 2.67 and 2.55 solar. Combined mag., colors. Capella is | first star for which an orbit was determined from interferometer measures, by Anderson at Mt. Wilson in 1920. Speckle | sep. 0.040" 1981.24 and 1981.68; 0.055" 1982.16. CPM with component H, a close binary, 10.0 dM1, 13.7 dM5 sep. 2" at | 723" from A, probably physical with A. Other components all faint and distant from A.
104.0204d, K 26.1k/s, V0 +29.5k/s, asini 37.3.
Hyades group.
Chromospheric He 10830 double. Balloon-borne spectrometer revealed pronounced emission of MgII. Soft X-ray emission. | Lithium content of the F-type component is 15 times that of the G component. Also classified G6III+F9III.
0.058".
CAPELLA; Alhajoth.
Diam. component A = 0.0052", component B = 0.0040".
16

Máquina del tiempo de la luz

17

Viaje Relativista

Cercanos en el cielo

Otros objetivos a pocos grados — mueve un poco el telescopio y sigue explorando.

Las puntuaciones de visibilidad asumen un Newton de 150 mm con Bortle 4.

}