SZ Piscium

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SZ Piscium

A visual band light curve for SZ Piscium, adapted from Eaton et al. (1982)[1]
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Pisces
Right ascension 23h 13m 23.778s[2]
Declination 02° 40′ 31.60″[2]
Apparent magnitude (V) 7.18[3]
Characteristics
Spectral type K1IV + F8V + ?[4]
Variable type
Distance
306 ± 5 ly
(94 ± 2 pc)
Semi-amplitude
(K1)
(primary)
74.2 km/s
Semi-amplitude (K2)
(secondary)
103.98 km/s
Details
K star
Rotational velocity (v sin i)
67.7±1.0[4] km/s
PPM 173881, WDS 23134+0241[7]
Database references
SIMBADdata

SZ Piscium is a suspected

light years based on parallax measurements.[2]

The variability of this star was reported by

subgiant in close orbit with an F8V main sequence star.[11] In 1972, H. L. Atkins and D. S. Hall included it on a list of RS Canum Venaticorum type variable systems and showed it has an infrared excess.[12]

Significant

star spot activity was found all over the K-type star, with variations in the total spot coverage observed over time.[6] It is estimated to be filling 85% of its Roche lobe due to the gravitational influence of the secondary. The rotation period of this star is several times slower than its orbital period, while the rotation of the F-type star is synchronous.[4] Changes in radial velocity of the system over time suggest it is a triple star system,[6] with the tertiary component having ~90% of the mass of the Sun and an orbital period of 1,283±10 days.[4]

References

Further reading