Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Auriga |
Right ascension | 04h 55m 45.84600s[1] |
Declination | +30° 33′ 04.2933″[1] |
Apparent magnitude (V) | 7.05[2] |
Characteristics | |
Evolutionary stage | Pre-main-sequence[3] |
Spectral type | A0Ve[4] |
U−B color index | +0.04[5] |
B−V color index | +0.11[5] |
Variable type | INA (Herbig Ae)[3][6] |
Astrometry | |
Radial velocity (Rv) | +8.9±0.9[7] km/s |
Proper motion (μ) | RA: +3.926[1] mas/yr Dec.: –24.112[1] mas/yr |
Parallax (π) | 6.1400 ± 0.0571 mas[1] |
Distance | 531 ± 5 ly (163 ± 2 pc) |
Details | |
Mass | 2.4±0.2[8] M☉ |
Radius | 2.5[9] R☉ |
Luminosity | ~38[8] L☉ |
Temperature | 9,772[10] K |
Age | 4±1[8] Myr |
Other designations | |
Database references | |
SIMBAD | data |
AB Aurigae is a young Herbig Ae star[3] in the Auriga constellation. It is located at a distance of approximately 531 light years from the Sun based on stellar parallax.[1] This pre-main-sequence star has a stellar classification of A0Ve,[4] matching an A-type main-sequence star with emission lines in the spectrum. It has 2.4 times the mass of the Sun and is radiating 38[8] times the Sun's luminosity from its photosphere at an effective temperature of 9,772 K.[10] The radio emission from the system suggests the presence of a thermal jet originating from the star with a velocity of 300 km s−1. This is causing an estimated mass loss of 1.7×10−8 M☉ yr−1.[8]
This star is known for hosting a dust disk that may harbour a condensing planet or brown dwarf. The star could host a possible substellar companion in wide orbit. The star is part of the young Taurus-Auriga association,[4] which is located in the Taurus Molecular Cloud.[12] The star itself may recently have encountered a dense cloudlet, which disrupted its debris disk and produced an additional reflection nebula.[13]
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