Theta Aurigae
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| Observation data Equinox J2000 |
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|---|---|
| Constellation | Auriga |
| Right ascension | 05h 59m 43.3s |
| Declination | +37° 12' 45" |
| Apparent magnitude (V) | +2.65 |
| Distance | 173 ± 7 ly (53 ± 2 pc) |
| Spectral type | A0pSi |
| Other designations | |
Theta Aurigae (θ Aur / θ Aurigae) is a binary star in the constellation Auriga. It is approximately 173 light-years from Earth. Rarely used proper names for this star include the Latin name Bogardus, and also the Arabic name Maha-Sim or Mahasim, which is a variant of the Arabic name Al-Mi'sam meaning "wrist" that was used to describe both Eta Aurigae and Theta Aurigae [1].
The primary, θ Aurigae A, is a white A-type main sequence dwarf with an apparent magnitude of +2.7. It's companion, θ Aurigae B, is a yellow G-type main sequence dwarf with an apparent magnitude of +7.2. The two stars are separated by 3.5 arcseconds. A third star, the 11th magnitude θ Aurigae C, is 49 arcseconds away, and is an optical companion.
The mean combined apparent magnitude of the system is +2.65 but the primary is an Alpha2 Canum Venaticorum type variable star so the system's brightness varies from magnitude +2.62 to +2.70 with a period of 1.37 days.
It is known as 五車四 ( the Fourth Star of the Five Chariots) in Chinese
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