Pi Hydrae

Pi Hydrae
Location of π Hydra (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Hydra
Right ascension 14h 06m 22.29749s
Declination −26° 40 56.5024
Apparent magnitude (V) 3.25
Characteristics
Spectral type K1 III–IV or K2-III Fe-0.5
U−B color index +1.040
B−V color index +1.120
Astrometry
Radial velocity (Rv)+26.7 km/s
Proper motion (μ) RA: +43.70 mas/yr
Dec.: 141.18 mas/yr
Parallax (π)32.30±0.16 mas
Distance101.0 ± 0.5 ly
(31.0 ± 0.2 pc)
Absolute magnitude (MV)0.79
Details
Mass1.40±0.21 M
Radius12.49±0.49 R
Luminosity60.8±2.6 L
Surface gravity (log g)2.40±0.11 cgs
Temperature4,565±75 K
Metallicity [Fe/H]−0.16±0.10 dex
Rotational velocity (v sin i)2.25 km/s
Age6.29±3.05 Gyr
Other designations
Markeb, π Hya, Pi Hya, 49 Hydrae, CPD−26°5170, FK5 519, HD 123123, HIP 68895, HR 5287, SAO 182244
Database references
SIMBADdata

Pi Hydrae, Latinized from π Hydrae, is a star in the constellation Hydra with an apparent visual magnitude of 3.3, making it visible to the naked eye. Parallax measurements put this star at a distance of about 101 light-years (31 parsecs) from the Earth.

The spectrum of this star shows it to have a stellar classification of K1 III-IV, with the luminosity class of 'III-IV' suggesting it is in an evolutionary transition stage somewhere between a subgiant and a giant star. It has a low projected rotational velocity of 2.25 km s−1. Pi Hydrae is radiating 61 times the Sun's luminosity from its outer envelope with an effective temperature of 4,565 K, giving it the orange hue of a K-type star.

Pi Hydrae is a type of giant known as a cyanogen-weak star, which means that its spectrum displays weak absorption lines of CN relative to the metallicity. (The last is a term astronomers use when describing the abundance of elements other than hydrogen and helium.) Otherwise, it appears to be a normal star of its evolutionary class, having undergone first dredge-up of nuclear fusion by-products onto its surface layers.