Nu Piscium

Star in the constellation Pisces From Wikipedia, the free encyclopedia

Nu Piscium (ν Piscium) is an orange-hued binary star[7] system in the zodiac constellation of Pisces. Prior to the formation of the modern constellation boundaries in 1930, it was designated 51 Ceti in the Cetus constellation.[8] Nu Piscium is visible to the naked eye, having a combined apparent visual magnitude of 4.44.[3] Based upon an annual parallax shift of 8.98 mas as seen from Earth,[2] it is located about 365 light years from the Sun.

Right ascension01h 41m 25.89414s[2]
Declination+05° 29′ 15.4018″[2]
Quick facts Constellation, Right ascension ...
ν Piscium
Location of ν Piscium (circled)
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Pisces[1]
Right ascension 01h 41m 25.89414s[2]
Declination +05° 29′ 15.4018″[2]
Apparent magnitude (V) 4.44[3]
Characteristics
Evolutionary stage red giant branch[2]
Spectral type K3 IIIb[3]
B−V color index 1.37[3]
Variable type Oscillating Red Giant
Astrometry
Radial velocity (Rv)0.6±0.18[2] km/s
Proper motion (μ) RA: âˆ’23.323 mas/yr[2]
Dec.: 3.505 mas/yr[2]
Parallax (π)8.9275±0.1567 mas[2]
Distance365 ± 6 ly
(112 ± 2 pc)
Absolute magnitude (MV)−0.78[1]
Details
ν Psc A
Mass1.66[3] M☉
Radius34.58+0.81
−0.83
[4] R☉
Luminosity380[3] L☉
Surface gravity (log g)1.91[5] cgs
Temperature4,154[3] K
Metallicity [Fe/H]−0.16[5] dex
Age3.41[3] Gyr
Other designations
ν Psc, 106 Piscium, BD+04°293, FK5 56, HD 10380, HIP 7884, HR 489, SAO 110065[6]
Database references
SIMBADdata
Close

The primary, component A, is an evolved, K-type giant star with a stellar classification of K3 IIIb.[3] It is a weak barium star, indicating that the atmosphere was previously enriched by accretion of s-process elements from what is now a white dwarf companion.[9] The giant has 1.66[3] times the mass of the Sun and has expanded to about 35[4] times the Sun's radius. It is about 3.4 billion years old and is radiating 380 times the Sun's luminosity from its photosphere at an effective temperature of 4,154 K.[3]

In 2026 the star was discovered to be an ORG (Oscillating Red Giant) variable by the Italian amateur research group GrAG (Gruppo Astrofili Galileo Galilei APS).[10]

Naming

In Chinese, 外屏 (Wài Píng), meaning Outer Fence, refers to an asterism consisting of ν Piscium, δ Piscium, ε Piscium, ζ Piscium, μ Piscium, ξ Piscium and α Piscium. Consequently, the Chinese name for ν Piscium itself is 外屏五 (Wài Píng wu, English: the Fifth Star of Outer Fence.)[11]

References

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