35 Piscium
From Wikipedia, the free encyclopedia
| Observation data Epoch J2000.0 |
|
|---|---|
| Constellation (pronunciation) |
Pisces |
| Right ascension | 00h 14m 58.820s |
| Declination | +8° 49' 15.06" |
| 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: 99.3 mas/yr Dec.: -37.0 mas/yr |
| Parallax (π) | 17 mas |
| Distance | 191.85669411765 ly (58.823529411765 pc) |
| Other designations | |
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.[2]
[edit] References
- ^ Simbad Query Result. Simbad. Retrieved on October 12, 2007.
- ^ P.C. Schmidtke (1980). "The Case for UU Piscium". International Amateur-Professional Photoelectric Photometry Communication 2: 19–20.
