Theta Piscium

Theta Piscium, Latinized from θ Piscium, is a single, orange-hued star in the zodiac constellation of Pisces, the fish. The annual parallax shift of this star was measured during the Hipparcos mission as 21.96 mas, which yields a distance estimate of about 149 light years. It is a faint star but visible to the naked eye with an apparent visual magnitude of 4.27. The star is moving away from the Sun with a radial velocity of +6 km/s.

Theta Piscium
Location of θ Piscium (circled)
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Pisces
Right ascension 23h 27m 58.09529s
Declination +6° 22 44.3720
Apparent magnitude (V) 4.27
Characteristics
Spectral type K1 III
U−B color index +1.00
B−V color index +1.062
Astrometry
Radial velocity (Rv)+6.05±0.19 km/s
Proper motion (μ) RA: −123.83 mas/yr
Dec.: −43.26 mas/yr
Parallax (π)21.96 ± 0.25 mas
Distance149 ± 2 ly
(45.5 ± 0.5 pc)
Absolute magnitude (MV)+0.83
Details
Mass1.58 M
Radius11 R
Luminosity51.3 L
Surface gravity (log g)2.70 cgs
Temperature4,684±23 K
Metallicity [Fe/H]0.06 dex
Rotational velocity (v sin i)3.1 km/s
Age2.45 Myr
Other designations
θ Psc, 10 Piscium, BD+05° 5173, FK5 1614, GC 32647, HD 220954, HIP 115830, HR 8916, SAO 128196, PPM 174110
Database references
SIMBADdata

At the estimated age of 2.5 billion years, this is an aging giant star with a stellar classification of K1 III, which means it has exhausted the supply of hydrogen at its core. It is a red clump star, indicating it is on the horizontal branch of its evolution and is generating energy through helium fusion at its core. Theta Piscium has 158% of the Sun's mass and its outer atmosphere has swollen to about 11 times the girth of the Sun. It is brighter yet cooler than the Sun, radiating 51.3 times the Sun's luminosity from its enlarged photosphere at an effective temperature of about 4,684 K.

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