HR 515

HR 515

Light curves for VY Piscium, adapted from Valtier et al. (1974). The vertical scale is hundredths of a magnitude.
Observation data
Epoch J2000      Equinox J2000
Constellation Pisces
Right ascension 01h 46m 35.29855s
Declination +17° 24 45.7125
Apparent magnitude (V) 6.54 - 6.59
Characteristics
Spectral type A8 III or F0V
B−V color index 0.256±0.010
Variable type δ Sct
Astrometry
Radial velocity (Rv)−1.0±4.4 km/s
Proper motion (μ) RA: +49.315 mas/yr
Dec.: +3.096 mas/yr
Parallax (π)6.4827±0.1220 mas
Distance503 ± 9 ly
(154 ± 3 pc)
Absolute magnitude (MV)+0.84
Details
Mass1.7 M
Radius4.7 R
Luminosity60 L
Surface gravity (log g)3.32 cgs
Temperature7,401 K
Metallicity [Fe/H]−0.02 dex
Rotational velocity (v sin i)96 km/s
Age944 Myr
Other designations
3 Arietis, VY Psc, BD+16°196, HD 10845, HIP 8271, HR 515, SAO 92622
Database references
SIMBADdata

HR 515 is a variable star in the zodiac constellation of Pisces, near the eastern constellation border with Aries. Before the constellation borders were officially set, it held the Flamsteed designation of 3 Arietis, abbreviated 3 Ari). This star has the variable star designation VY Piscium, or VY Psc for short. It is a white-hued star that is near the lower limit of visibility to the naked eye with an apparent visual magnitude that ranges from 6.54 down to 6.59. Parallax measurements provide a distance estimate of approximately 503 light years from the Sun.

Gray and associates (1989) found a stellar classification of A8 III for this object, matching an evolved A-type giant star. Abt and Morrell (1995) listed a class of F0V, suggesting it is an F-type main-sequence star. It is a Delta Scuti variable whose brightness varies between magnitudes 6.54 and 6.59 with a period of 0.219 days. The star shows a high rate of spin with a projected rotational velocity of 96 km/s. It has 4.7 times the size of the Sun and is radiating 60 times the Sun's luminosity from its photosphere at an effective temperature of 7,401 K.