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B3 Hydrae

Multiple star system in the constellation Hydra From Wikipedia, the free encyclopedia

b3 Hydrae (6 Crateris) is a star in the constellation Hydra at a distance of approximately 98 light-years (about 30 parsecs) from the Sun. It has three optical companions, which are background stars located much farther away.

Quick facts Constellation, Right ascension ...
b3 Hydrae
Observation data
Epoch J2000.0      Equinox ICRS
Constellation Hydra[1]
Right ascension 10h 53m 29.532s[2]
Declination −20° 08 19.43[2]
Apparent magnitude (V) 5.24[3]
Characteristics
Evolutionary stage main sequence[2]
Spectral type F5V[3]
U−B color index +0.06[3]
B−V color index +0.47[3]
Astrometry
Radial velocity (Rv)−4.08±0.12[2] km/s
Proper motion (μ) RA: +80.915[2] mas/yr
Dec.: −238.566[2] mas/yr
Parallax (π)33.2327±0.1234 mas[2]
Distance98.1 ± 0.4 ly
(30.1 ± 0.1 pc)
Absolute magnitude (MV)+2.79[1]
Details
Mass1.48[4] M
Radius1.93[5] R
Luminosity6.02[5] L
Surface gravity (log g)3.99[5] cgs
Temperature6,505[5] K
Metallicity [Fe/H]+0.09[4] dex
Rotation27.1 days[6]
Rotational velocity (v sin i)6.0[7] km/s
Age2.27[4] Gyr
Other designations
b3 Hya, 6 Crt, HD 94388, HIP 53252, HR 4521, SAO 156301, PPM 258261, CCDM J10534-2009A, WDS J10535-2008A[8]
Database references
SIMBADdata
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Description

b3 Hydrae (WDS J10535-2008A) is a yellow-white main sequence star with the spectral type of F5V. The apparent magnitude of the star is +5.232. It has about 1.5 M, its radius is about 1.9 R and the luminosity is about 6.0 L. The age of the star is determined to be about 1.647 billion years.[4] The effective temperature is about 6,505 K.

Optical companions

BD−19 3124

The secondary (BD−19 3124) is a yellow main sequence star of spectral type G5.[9] The apparent magnitude of the star is +9.6.[10] The mass is about 1.492 ± 0.001 M[11], the radius is about 2.071 ± 0.008 R[11], the luminosity is about 6.946 ± 0.001 L[11]. The effective temperature is about 6,566±1 K[11]. It is 119.6 arcseconds away from b3 Hydrae[12] and about 774 light-years (237 parsecs) away from the Solar System.[11]

UCAC2 23866861

The third component (UCAC2 23866861) is a yellow dwarf of spectral type G.[citation needed] The apparent magnitude of the star is +11.6.[13] The mass is about 0.989 ± 0.001 M[14], the radius is about 1.315 ± 0.002 R[14], the luminosity is about 1.662 ± 0.001 L[14]. The effective temperature is about 5,761±4 K[14]. It is separated from BD−19 3124 by 13.7 arc seconds[12] and is about 850 light-years (260 parsecs) away from the Solar System.[14]

UCAC2 23866855

The fourth component (UCAC2 23866855) is a yellow-white star of spectral type F.[citation needed] The apparent magnitude of the star is +13.5.[15] The mass is about 1.332 ± 0.001 M[16] the radius is about 1.829 ± 0.005 R[16] the luminosity is about 4.356 ± 0.001 L[16] the effective temperature is about 6,236±1 K[16]. It is located 40.5 arc seconds away from BD−19 3124[12] and is about 3,820 light-years (1,170 parsecs) away from the Solar System.[16]

References

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