Capella (Alpha Aurigae)
An infrared image of the double star Capella, from an array of telescopes. Credit: COAST / MRAO Cambridge.
Capella is a multiple system in which the dominant components are two post-main-sequence G-type stars, each with roughly the same temperature as the Sun, a radius of about 10 times that of the Sun, and a mass of 2.5 solar masses. One has a luminosity of 50 times that of the Sun, the other of 80 times. This pair, separable only by spectroscope, lie less than 100 million kilometers apart and orbit each other every 104.02 days.
Capella is a source of X-rays, probably because of surface magnetic activity similar to that seen on the Sun, but which star is responsible is uncertain. Capella also has a faint companion that is itself a double, made of two dim red dwarf M stars, that orbits almost a light-year away from the main pair.
|visual magnitude||+0.08 (combined); +0.71/+0.96|
|absolute magnitude||-0.48 (combined); +0.14/+0.19|
|spectral types||G8III + G0III + M5V|
|distance||42.2 light-years (19.5 pc)|
|position||R.A. 05h 16m 41.4s,
Dec. +45° 59' 53"
|other designations||Alhajoth, 13 Aurigae,
HR 1708, HD 34029, Gl 194,
BD+45°1077, FK5 193, HIP 24608,
SAO 40186, GC 6427, ADS 3841,