HD 204521

HD 204521
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
Declination +70° 28 39.1434
Apparent magnitude (V) 7.26 (binoculars)
Characteristics
Spectral type G0V
B−V color index 0.619±0.015
Astrometry
Radial velocity (Rv)−76.78±0.12 km/s
Proper motion (μ) RA: +40.632 mas/yr
Dec.: +39.411 mas/yr
Parallax (π)37.9375±0.0155 mas
Distance85.97 ± 0.04 ly
(26.36 ± 0.01 pc)
Absolute magnitude (MV)5.15
Details
Mass0.77±0.03 or 0.997 M
Radius0.92 R
Luminosity0.76 L
Surface gravity (log g)4.43±0.02 cgs
Temperature5,699±50 K
Metallicity [Fe/H]−0.75±0.05 dex
Rotational velocity (v sin i)3.6 km/s
Age8.43±4.24 Gyr
Other designations
BD+69°1169, GJ 4194, HD 204521, HIP 105766, SAO 10045, TYC 4465-1133-1
Database references
SIMBADdata

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. It is located at a distance of 86 light years from the Sun based on parallax, and has an absolute magnitude of 5.15. The star is drifting closer with a radial velocity of −77 km/s, and is predicted to come to within 7.96 light-years in 334,000 years. At that distance the star can have a relatively small perturbing effect on comets in the Oort cloud.

This is an ordinary G-type main-sequence star with a stellar classification of G0V, indicating that it is generating energy through core hydrogen fusion. It is roughly 8 billion years old and appears metal-deficient. 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.