52 Arietis
Observation data Epoch J2000 Equinox J2000 |
|
---|---|
Constellation | Aries |
Right ascension | 03h 05m 26.68819s[1] |
Declination | +25° 15′ 18.6257″[1] |
Apparent magnitude (V) | 5.46[2] |
Characteristics | |
Spectral type | B7 V + B7 V[3] |
U−B color index | -0.38[2] |
B−V color index | -0.03[2] |
Astrometry | |
Radial velocity (Rv) | 9[4] km/s |
Proper motion (μ) | RA: +1.44[1] mas/yr Dec.: -10.26[1] mas/yr |
Parallax (π) | 6.05 ± 1.06[1] mas |
Distance | approx. 540 ly (approx. 170 pc) |
Orbit | |
Primary | 52 Ari A |
Companion | 52 Ari B |
Period (P) | 227[5] yr |
Semi-major axis (a) | 0.47" |
Eccentricity (e) | 0.73[5] |
Inclination (i) | 77.5° |
Longitude of the node (Ω) | 92.8° |
Periastron epoch (T) | 1938.5 |
Details | |
52 Ari A | |
Mass | 5.12[6] M☉ |
Radius | 3.3[7] R☉ |
Luminosity | 452[8] L☉ |
Temperature | 12,912[8] K |
Rotational velocity (v sin i) | 159[8] km/s |
52 Ari B | |
Mass | 5.12[6] M☉ |
Other designations | |
52 Ari A: HD 19134, HR 927. | |
52 Ari B: HD 19135, HR 928. |
52 Arietis (abbreviated 52 Ari) is a triple star system in the northern constellation of Aries. 52 Arietis is the Flamsteed designation. The combined apparent magnitude is +5.46,[2] which is bright enough to be faintly visible to the naked eye. Based upon an annual parallax shift of 6.05 mas,[1] the system is roughly 540 light-years (170 parsecs) distant from the Earth. The inner pair of this system consist of two nearly identical B-type main sequence stars, each with about five times the mass of the Sun. The tertiary component is a smaller star with 88% of the Sun's mass.[6]
References
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External links
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