43 Persei

43 Persei
Location of 43 Persei (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Perseus
Right ascension 03h 56m 36.52069s
Declination +50° 41 43.3646
Apparent magnitude (V) 5.28
Characteristics
Spectral type F5V
U−B color index +0.00
B−V color index +0.41
Astrometry
Radial velocity (Rv)+39.10 km/s
Proper motion (μ) RA: +92.450 mas/yr
Dec.: -129.755 mas/yr
Parallax (π)26.0059±0.1271 mas
Distance125.4 ± 0.6 ly
(38.5 ± 0.2 pc)
Absolute magnitude (MV)2.23
Orbit
Period (P)30.438 days
Semi-major axis (a) 16 Gm (0.11 AU)
Eccentricity (e)0.631
Periastron epoch (T)2,440,873.14 JD
Argument of periastron (ω)
(secondary)
27.07°
Semi-amplitude (K1)
(primary)
51.85 km/s
Semi-amplitude (K2)
(secondary)
54.40 km/s
Details
Mass1.54 M
Radius2.4 R
Luminosity10.81 L
Surface gravity (log g)4.12 cgs
Temperature6,609 K
Metallicity [Fe/H]0.00 dex
Rotational velocity (v sin i)17 km/s
Other designations
A Persei, 43 Per, BD+50°860, GC 4728, HD 24546, HIP 18453, HR 1210, SAO 24314, CCDM J03566+5042AP, WDS J03566+5042AD
Database references
SIMBADdata

43 Persei is a binary star system in the northern constellation Perseus. It is visible to the naked eye as a dim, yellow-white hued star with an apparent visual magnitude of 5.28. The system is located around 38.5 parsecs (125.4 ly) distant from the Sun, based on parallax.

This is a double-lined spectroscopic binary with an orbital period of 30.4 days and an eccentricity of 0.6. The primary component is an F-type main-sequence star with a stellar classification of F5V, a star that is fusing its core hydrogen. It has 1.54 times the mass of the Sun, 2.4 times the Sun's radius, and is spinning with a projected rotational velocity of 17 km/s (11 mi/s). The star shines 10.8 times brighter than the Sun at an effective temperature of 6,609 K (6,336 °C; 11,437 °F).

There are distant companions B (separation 75.5" and magnitude 10.66), C (separation 85.6" and magnitude 12.18), and D (separation 68" and magnitude 13.43).