Location of HD 204521; not visible on this chart, but just to the west of β Cephei (circled) | |
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Cepheus |
Right ascension | 21h 25m 16.79696s[1] |
Declination | +70° 28′ 39.1434″[1] |
Apparent magnitude (V) | 7.26[2] (binoculars) |
Characteristics | |
Spectral type | G0V[3] |
B−V color index | 0.619±0.015[2] |
Astrometry | |
Radial velocity (Rv) | −76.78±0.12[1] km/s |
Proper motion (μ) | RA: +40.632[1] mas/yr Dec.: +39.411[1] mas/yr |
Parallax (π) | 37.9375 ± 0.0155 mas[1] |
Distance | 85.97 ± 0.04 ly (26.36 ± 0.01 pc) |
Absolute magnitude (MV) | 5.15[2] |
Details | |
Mass | 0.77±0.03[4] or 0.997[5] M☉ |
Radius | 0.92[1] R☉ |
Luminosity | 0.76[1] L☉ |
Surface gravity (log g) | 4.43±0.02[4] cgs |
Temperature | 5,699±50[4] K |
Metallicity [Fe/H] | −0.75±0.05[4] dex |
Rotational velocity (v sin i) | 3.6[6] km/s |
Age | 8.43±4.24[7] Gyr |
Other designations | |
Database references | |
SIMBAD | data |
HD 204521 is a star in the northern constellation of Cepheus. In the sky it positioned just to the west of the magnitude 3.2 star Beta Cephei (β Cep). This object has a yellow hue similar to the Sun but is too faint to be visible to the naked eye with an apparent visual magnitude of 7.26.[2] It is located at a distance of 86 light years from the Sun based on parallax, and has an absolute magnitude of 5.15.[2] The star is drifting closer with a radial velocity of −77 km/s,[2] and is predicted to come to within 7.96 light-years in 334,000 years.[5] At that distance the star can have a relatively small perturbing effect on comets in the Oort cloud.[9]
This is an ordinary G-type main-sequence star with a stellar classification of G0V,[3] indicating that it is generating energy through core hydrogen fusion. It is roughly 8 billion years old[7] and appears metal-deficient.[10] The mass of this star appears to be at or below that of the Sun, and it is radiating 76% of the Sun's luminosity from its photosphere at an effective temperature of 5,699 K.[4]
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