Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Aries |
Right ascension | 01h 57m 55.71647s[1] |
Declination | +23° 35′ 45.8295″[1] |
Apparent magnitude (V) | 4.79[2] (4.95/7.75)[3] |
Characteristics | |
Spectral type | F0 V + G1 V[3] |
U−B color index | +0.09[2] |
B−V color index | +0.28[2] |
R−I color index | 0.16 |
Astrometry | |
Radial velocity (Rv) | -1.4[4] km/s |
Proper motion (μ) | RA: -92.55[1] mas/yr Dec.: -13.25[1] mas/yr |
Parallax (π) | 25.32 ± 0.30 mas[1] |
Distance | 129 ± 2 ly (39.5 ± 0.5 pc) |
Details | |
λ Ari A | |
Surface gravity (log g) | 3.88[5] cgs |
Temperature | 7,177[5] K |
Metallicity [Fe/H] | +0.01[5] dex |
Rotational velocity (v sin i) | 107[6] km/s |
λ Ari B | |
Surface gravity (log g) | 3.88[5] cgs |
Temperature | 5,929[5] K |
Metallicity [Fe/H] | –0.03[5] dex |
Other designations | |
Database references | |
SIMBAD | data |
Lambda Arietis (λ Ari, λ Arietis) is the Bayer designation for a double star in the northern constellation of Aries. Based upon an annual parallax shift of 25.32 arcseconds, this system is approximately 129 light-years (40 parsecs) distant from Earth. The pair have a combined apparent visual magnitude of 4.79,[2] which is bright enough to be viewed with the naked eye. Because the yellow secondary is nearly three magnitudes fainter than the white primary, they are a challenge to split with quality 7× binoculars and are readily resolvable at 10×.[8]
The brighter component is an F-type main sequence star with a visual magnitude of 4.95 and a stellar classification of F0 V.[3] At an angular separation of 37.4 arcseconds is fainter, magnitude 7.75 companion. This is a G-type main sequence star with a classification of G1 V.[3]
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