Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Hydra |
Right ascension | 14h 28m 10.42638s[1] |
Declination | −29° 29′ 29.8884″[1] |
Apparent magnitude (V) | 4.97[2] (5.70 + 5.70 + 10.00)[3] |
Characteristics | |
Evolutionary stage | main sequence[4] |
Spectral type | B7/8V[5] |
B−V color index | −0.074±0.003[2] |
Astrometry | |
Radial velocity (Rv) | 5.4±3.8[2] km/s |
Proper motion (μ) | RA: −25.23[1] mas/yr Dec.: −23.03[1] mas/yr |
Parallax (π) | 8.29 ± 0.28 mas[1] |
Distance | 390 ± 10 ly (121 ± 4 pc) |
Absolute magnitude (MV) | −0.43[2] |
Details | |
52 Hya A | |
Mass | 3.82±0.06[4] M☉ |
Luminosity | 310.5+24.5 −22.8[4] L☉ |
Temperature | 12,853±89[4] K |
Rotational velocity (v sin i) | 204[4] km/s |
Other designations | |
Database references | |
SIMBAD | data |
52 Hydrae is a triple star system[7] in the constellation Hydra. It has the Bayer designation l Hydrae; 52 Hydrae is the Flamsteed designation.[6] This system is visible to the naked eye as a faint, blue-white hued star with an apparent visual magnitude of 4.97.[2] It is a probable (80% chance) member of the Sco OB2 moving group of stars,[8] and is moving away from the Earth with a heliocentric radial velocity of 5 km/s.[2]
The primary component is a binary system[7] consisting of two nearly equal components with an orbital period of around 15 years[9] and an angular separation of 0.1″.[7] It shows a combined stellar classification of B7/8V,[5] which matches a B-type main-sequence star. The third component is a magnitude 10.0 star at a separation of 4.2″[7] with a mass similar to the Sun. It is orbiting the inner pair with a period of around 3,900 years.[9]
vanLeeuwen2007
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was invoked but never defined (see the help page).Rizzuto2011
was invoked but never defined (see the help page).Tokovinin2008
was invoked but never defined (see the help page).