35 Piscium

35 Piscium[1]
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Pisces
Right ascension 00h 14m 58.84s [2]
Declination +08° 49 15.5 [2]
Apparent magnitude (V) 6.01
Characteristics
Spectral type F0IV+...
U−B color index +0.04
B−V color index +0.32
Astrometry
Radial velocity (Rv)0.9 km/s
Proper motion (μ) RA: 99.42 ± 0.96 [2] mas/yr
Dec.: -23.62 ± 0.67 [2] mas/yr
Parallax (π)12.86 ± 1.05[2] mas
Distance250 ± 20 ly
(78 ± 6 pc)
Other designations
35 Piscium, UU Piscum, HR 50, BD+08° 19, HD 1061, SAO 109087, GC 287, HIP 1196

35 Piscium is a binary star system in the constellation Pisces. According to Cester (1960), the system has a period of 0.841658 days, zero eccentricity, and an inclination of 19 degrees. Although thought to be an eclipsing binary, Cester argued that the apparent eclipses are not real, and were caused by seeing different portions of distorted-shaped stars in a near contact binary system.[3]

References

  1. "Simbad Query Result". Simbad. Retrieved October 12, 2007.
  2. 2.0 2.1 2.2 2.3 2.4 van Leeuwen, F. (2007). "HIP 1196". Hipparcos, the New Reduction. Retrieved 2010-08-23.
  3. P.C. Schmidtke (1980). "The Case for UU Piscium". International Amateur-Professional Photoelectric Photometry Communication 2: 19–20. Bibcode:1980IAPPP...2...19S.