Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Pegasus |
Right ascension | 23h 08m 51.186s[2] |
Declination | +17° 12′ 56.00″[2] |
Apparent magnitude (V) | 9.95 – 10.62[3] |
Characteristics | |
Spectral type | A3 to F1[4] |
Variable type | SX Phe[5][3] |
Astrometry | |
Radial velocity (Rv) | −25.30±2.7[6] km/s |
Proper motion (μ) | RA: 47.248 mas/yr[2] Dec.: −22.103 mas/yr[2] |
Parallax (π) | 2.4588 ± 0.0452 mas[2] |
Distance | 1,330 ± 20 ly (407 ± 7 pc) |
Absolute magnitude (MV) | 2.34[7] 0.84[8] |
Orbit[5] | |
Period (P) | 15,425.0±205.7 d |
Semi-major axis (a) | ≥ 0.254±0.034 AU |
Eccentricity (e) | 0.65 ± 0.10 |
Periastron epoch (T) | 2438276.86149 ± 0.00013 HJD |
Details | |
Mass | 1.54 M☉[7] 1.40[8] M☉ |
Radius | 2.09±0.25 R☉[4] 3.74 – 3.95[8] R☉ |
Luminosity | 11.34+2.82 −2.51 L☉[4] 34.6±2.1[8] L☉ |
Temperature | 7,660 K[7] (7,950 – 6,750)[9] K |
Metallicity [Fe/H] | −0.56[5] dex |
Rotational velocity (v sin i) | 23.6[5] km/s |
Age | 1.7[7] Gyr |
Other designations | |
Database references | |
SIMBAD | data |
DY Pegasi, abbreviated DY Peg, is a binary star[5] system in the northern constellation of Pegasus. It is a well-studied[11] SX Phoenicis variable star with a brightness that ranges from an apparent visual magnitude of 9.95 down to 10.62 with a period of 1.75 hours.[3] This system is much too faint to be seen with the naked eye, but can be viewed with large binoculars or a telescope.[12] Based on its high space motion and low abundances of heavier elements, it is a population II star system.[13]
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