Upsilon1 Hydrae

Upsilon1 Hydrae (υ1 Hydrae, abbreviated Ups1 Hya, υ1 Hya), also named Zhang, is a yellow-hued star in the constellation of Hydra.

It is visible to the naked eye, having an apparent visual magnitude of 4.12. Based upon an annual parallax shift of 12.36 mas as seen from Earth, it is located about 264 light-years from the Sun. The star is moving closer to the Sun with a radial velocity of −14.34 km/s. In 2005 it was announced that it had a substellar companion.

Upsilon1 Hydrae
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Hydra
Right ascension 09h 51m 28.69384s
Declination −14° 50′ 47.7710″
Apparent magnitude (V) 4.12
Characteristics
Spectral type G6/8III
U−B color index +0.65
B−V color index +0.92
Astrometry
Radial velocity (Rv)−14.34 km/s
Proper motion (μ) RA: +18.88 mas/yr
Dec.: −21.85 mas/yr
Parallax (π)12.36 ± 0.26 mas
Distance264 ± 6 ly
(81 ± 2 pc)
Absolute magnitude (MV)−0.43
Details
Mass3.33 M
Radius14.69 R
Luminosity162 L
Surface gravity (log g)2.95 cgs
Temperature5,185 K
Metallicity [Fe/H]0.10 dex
Rotational velocity (v sin i)2.11 km/s
Age270 Myr
Other designations
Zhang, upsilon1 Hya, 39 Hydrae, BD-14°2963, HD 85444, HIP 48356, HR 3903, SAO 155542
Database references
SIMBADdata

Nomenclature

υ1 Hydrae (Latinised to Upsilon1 Hydrae) is the star's Bayer designation.

In Chinese, 張宿 (Zhāng Sù), meaning Extended Net, refers to an asterism consisting of Upsilon1 Hydrae, Lambda Hydrae, Mu Hydrae, HD 87344, Kappa Hydrae and Phi1 Hydrae. Consequently, Upsilon1 Hydrae itself is known as 張宿一 (Zhāng Sù yī), "the First Star of Extended Net". In 2016, the International Astronomical Union (IAU) organized a Working Group on Star Names (WGSN) to catalog and standardize proper names for stars. The WGSN approved the name Zhang for this star on 30 June 2017 and it is now so included in the List of IAU-approved Star Names.

Properties

With a stellar classification of G6/8 III, Upsilon1 Hydrae is an evolved G-type giant star. It has an estimated 3.3 times the mass of the Sun and has expanded to 14.7 times the Sun's radius. The star is about 270 million years old with a projected rotational velocity of just 2.11 km/s. It is radiating 162 times the Sun's luminosity from its photosphere at an effective temperature of 5,185 K.

Substellar companion

The Okayama Planet Search team published a paper in 2005 reporting investigations on radial velocity variations observed for a set of class G giants and announcing the detection of a brown dwarf companion in orbit around Upsilon1 Hydrae. The orbital period for this companion is roughly 4.1 years, and it has a high eccentricity of 0.57. Since the inclination of the orbit to the line-of-sight is unknown, only a lower bound on the mass can be determined. It has at least 49 times the mass of Jupiter.

The Upsilon1 Hydrae planetary system
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
b ≥49 MJ 3.9 1,500 0.57

References

Tags:

Upsilon1 Hydrae NomenclatureUpsilon1 Hydrae PropertiesUpsilon1 HydraeApparent visual magnitudeConstellationHydra (constellation)Light-yearMilliarcsecondRadial velocityStarStellar parallaxSun

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