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Nu Hydrae

Nu Hydrae
Diagram showing star positions and boundaries of the Hydra constellation and its surroundings
Cercle rouge 100%.svg

Location of ν Hydra (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Hydra
Right ascension 10h 49m 37.48875s
Declination –16° 11′ 37.1360″
Apparent magnitude (V) 3.115
Characteristics
Spectral type K0/K1 III
U−B color index +1.305
B−V color index +1.239
Astrometry
Radial velocity (Rv) –1.2 km/s
Proper motion (μ) RA: +93.35 mas/yr
Dec.: +198.88 mas/yr
Parallax (π) 22.69 ± 0.23mas
Distance 144 ± 1 ly
(44.1 ± 0.4 pc)
Details
Mass 2.0 M
Radius 21 R
Luminosity 151 L
Surface gravity (log g) 2.3 cgs
Temperature 4,335 K
Metallicity [Fe/H] –0.30 dex
Rotational velocity (v sin i) 5.3 km/s
Other designations
43 Hydrae, HD 93813, HR 4232, SAO 156256, FK5 410, BD-15 3138, HIP 52943.
Database references
SIMBAD data

Nu Hydrae (ν Hya, ν Hydrae) is a star in the constellation Hydra, near the border with the neighboring constellation of Crater. It has an apparent visual magnitude of 3.115, which is bright enough to be seen with the naked eye. Based upon parallax measurements, this star is located at a distance of about 144 light-years (44 parsecs) from the Earth.

The spectrum of this star matches a stellar classification of K0/K1 III, where the luminosity class of 'III' indicates this is a giant star that has exhausted the supply of hydrogen at its core and evolved away from the main sequence. The radius of this star has expanded to 21 times the Sun's radius with an emission of about 151 times the luminosity of the Sun. This expanded outer envelope has an effective temperature of about 4,335 K, giving it the characteristic orange hue of a K-type star.

Nu Hydrae is an X-ray emitter with an estimated luminosity of 6.6 × 1028erg s−1 in the X-ray band. The abundance of elements other than hydrogen and helium, what astronomers term the star's metallicity, is about half that in the Sun. It has a relatively high proper motion across the celestial sphere, suggesting that it has a peculiar velocity roughly three times higher than its neighbors.


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