HD 1976

HD 1976
Location of HD 1976 (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Cassiopeia
Right ascension 00h 24m 15.65400s
Declination +52° 01 11.7032
Apparent magnitude (V) 5.580 (combined)
Characteristics
Spectral type (B5IV + unknown) + ~B5-6IV
U−B color index −0.619
B−V color index −0.121
J−H color index −0.102
J−K color index −0.106
Variable type Slowly pulsating B-type star (A; disputed)
Astrometry
Radial velocity (Rv)−9.70±0.49 km/s
Proper motion (μ) RA: 15.504 mas/yr
Dec.: −4.061 mas/yr
Parallax (π)2.4621±0.33 mas
Distanceapprox. 1,300 ly
(approx. 410 pc)
Orbit
PrimaryHD 1976 Aa
CompanionHD 1976 Ab
Period (P)25.4163±0.0008 d
Semi-major axis (a)0.42±0.05 mas
Eccentricity (e)0.05±0.03
Inclination (i)100.7±1.2°
Longitude of the node (Ω)339.9±1.1°
Periastron epoch (T)59477±5
Argument of periastron (ω)
(secondary)
61±52°
Orbit
PrimaryHD 1976 A
CompanionHD 1976 B
Period (P)171±3 yr
Semi-major axis (a)208.0±2.7 mas
Eccentricity (e)0.162±0.008
Inclination (i)62.8±0.4°
Longitude of the node (Ω)27.8±0.4°
Periastron epoch (T)33710±679
Argument of periastron (ω)
(secondary)
306.0±4°
Details
HD 1976 Aa
Mass6.45±0.17, 6.348 M
Radius5.24+0.14
−0.10
 R
Surface gravity (log g)3.81±0.01 cgs
Temperature16526+100
−82
 K
Rotational velocity (v sin i)170±4 km/s
Age~60 Myr
HD 1976 Ab
Mass1.83, 4.0±0.7 M
Radius1.83 R
Surface gravity (log g)4.18 cgs
Temperature8071+266
−352
 K
Rotational velocity (v sin i)165 km/s
HD 1976 B
Mass6.10+0.27
−0.26
 M
Radius4.48±0.20 R
Surface gravity (log g)3.92±0.02 cgs
Temperature13620+154
−144
 K
Rotational velocity (v sin i)73+6
−5
 km/s
Other designations
V746 Cassiopeiae, AG+51°39, BD+51°62, Gaia DR3 418916648901801728, GC 476, HD 1976, HIP 1921, HR 91, SAO 21366, PPM 25297, WDS J00243+5201AB, TIC 202418751, TYC 3260-2342-1, GSC 03260-02342, 2MASS J00241564+5201119, ADS 328
Database references
SIMBADHD 1976

HD 1976 is a hierarchical triple system in the deep northern constellation of Cassiopeia, somewhere around 1,100 light-years (340 parsecs) from Earth. It has the variable-star designation V746 Cassiopeiae (abbreviated to V746 Cas). The system is faintly visible to the naked eye under dark skies, having an apparent magnitude of 5.580. It consists of an inner pair between a B-type subgiant and a less massive unknown-type star, which is distantly orbited by another B-type subgiant. It is currently moving closer towards the Solar System at a heliocentric radial velocity of −9.70 km/s.