Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Perseus |
Right ascension | 02h 35m 17.127s[1] |
Declination | +56° 08′ 44.72″[1] |
Apparent magnitude (V) | 10.5 - 16.0[2] |
Characteristics | |
Spectral type | C5,4pJ:[3] C-R4+ C25.5[4] |
B−V color index | 1.79[5] |
V−R color index | 1.12[5] |
J−H color index | 0.185[6] |
J−K color index | 1.963[6] |
Variable type | DY Per[7] |
Astrometry | |
Radial velocity (Rv) | −38[8] km/s |
Proper motion (μ) | RA: +2.264[1] mas/yr Dec.: −0.675[1] mas/yr |
Parallax (π) | 0.6718 ± 0.0251 mas[1] |
Distance | 1,500[9] pc |
Absolute magnitude (MV) | −2.5 (max)[7] |
Details | |
Radius | 87[10] R☉ |
Luminosity | 522[11] L☉ |
Surface gravity (log g) | 0.0[12] cgs |
Temperature | 2,900-3,100[12] K |
Metallicity [Fe/H] | −2.0 to −0.5[12] dex |
Other designations | |
Database references | |
SIMBAD | data |
DY Persei is a variable star and carbon star in the Perseus constellation. At maximum it is 11th magnitude and at its faintest it drops to 16th magnitude. DY Persei is the prototype of the very rare DY Persei class of variables that pulsate like red variables but also fade from sight like R Coronae Borealis variables.
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