Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Delphinus |
Right ascension | 20h 49m 59.0925s[1] |
Declination | +05° 32′ 40.5081″[1] |
Apparent magnitude (V) | 6.19±0.01[2] |
Characteristics | |
Spectral type | K0[3] |
U−B color index | +0.79[4] |
B−V color index | +0.98[4] |
Astrometry | |
Radial velocity (Rv) | −21.63±0.31[5] km/s |
Proper motion (μ) | RA: +43.408 mas/yr[1] Dec.: −0.174 mas/yr[1] |
Parallax (π) | 8.2537 ± 0.1261 mas[1] |
Distance | 395 ± 6 ly (121 ± 2 pc) |
Absolute magnitude (MV) | +0.7[6] |
Details | |
Mass | 3.12[7] M☉ |
Radius | 10.54[8] R☉ |
Luminosity | 56.3[9] L☉ |
Surface gravity (log g) | 2.8[7] cgs |
Temperature | 4,809[10] K |
Metallicity [Fe/H] | +0.17[7] dex |
Other designations | |
Database references | |
SIMBAD | data |
HD 198404 (HR 7975) is a star in the equatorial constellation Delphinus. It has an apparent magnitude of 6.19,[2] allowing it to be faintly seen with the naked eye. Parallax measurements place the object at a distance of 395 light years[1] and it is approaching the Solar System with a heliocentric radial velocity of −21.6 km/s.[5]
HD 198404 has a simple stellar classification of K0,[3] indicating that it is a K-type star. Its enlarged diameter of 10.54 R☉[8] and its low surface gravity[7] suggest that it has evolved away from the main sequence to become a giant star.[7] HD 198404 has 3.12 times the mass of the Sun[7] and radiates at 56 times the luminosity of the Sun[9] from its photosphere at an effective temperature of 4,809 K,[10] giving it a yellowish orange hue. The star is metal enriched, having an iron abundance 48% greater than that of the Sun.[7]
HD 198404 has an optical companion located 78.2″ away along a position angle of 127° (as of 2014).[13]
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