16 Persei

16 Persei
Location of 16 Persei (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Perseus
Right ascension 02h 50m 35.05979s
Declination 38° 19 07.1080
Apparent magnitude (V) 4.22
Characteristics
Spectral type F2III
U−B color index +0.08
B−V color index +0.34
Variable type δ Sct(?)
Astrometry
Radial velocity (Rv)+14.00 km/s
Proper motion (μ) RA: +195.77 mas/yr
Dec.: −109.98 mas/yr
Parallax (π)27.01±0.19 mas
Distance120.8 ± 0.8 ly
(37.0 ± 0.3 pc)
Absolute magnitude (MV)1.38
Details
Mass1.80 M
Radius3.2 R
Luminosity23.36 L
Surface gravity (log g)3.72 cgs
Temperature7,004 K
Metallicity [Fe/H]−0.04 dex
Rotational velocity (v sin i)149 km/s
Age1.44 Gyr
Other designations
16 Per, NSV 956, BD+37°646, FK5 2194, GC 3401, HD 17584, HIP 13254, HR 840, SAO 55928, CCDM J02506+3818A, LTT 10924
Database references
SIMBADdata

16 Persei is a single, suspected variable star in the northern constellation of Perseus, located approximately 121 light years away based on parallax. It is visible to the naked eye as a yellow-white hued star with an apparent visual magnitude of 4.22. This object is moving further from the Earth with a heliocentric radial velocity of +14 km/s. It displays a relatively high proper motion, traversing the celestial sphere at the rate of 0.224 per year.

Based upon a stellar classification of F2 III, this matches an aging giant star that has exhausted the hydrogen at its core and is evolving away from the main sequence. It is a possible pulsating Delta Scuti variable, although there is some uncertainty about this classification. However, Kunzli and North (1998) found no variation. The star is 1.44 billion years old with 1.8 times the mass of the Sun and 3.2 times the Sun's radius. It shows a high rotation rate with a projected rotational velocity of 149 km/s, which is causing an equatorial bulge that is an estimated 24% larger than the polar radius. 16 Persei is radiating 23 times the Sun's luminosity from its photosphere at an effective temperature of 7,004 K.

It has two reported visual companions: B, with a magnitude of 12.8 and separation of 76.7", and C, with magnitude 10.43 and separation 234".