Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Andromeda |
HD 224635 | |
Right ascension | 23h 59m 29.2915s[1] |
Declination | +33° 43′ 25.8773″[1] |
Apparent magnitude (V) | 6.46[2] |
HD 224636 | |
Right ascension | 23h 59m 29.2054s[3] |
Declination | +33° 43′ 27.6539″[3] |
Apparent magnitude (V) | 6.72[2] |
Characteristics | |
HD 224635 | |
Spectral type | F8[4] |
B−V color index | 0.51[5] |
HD 224636 | |
Spectral type | G1[4] |
B−V color index | 0.55[5] |
Astrometry | |
Radial velocity (Rv) | −7.90±0.2[6] km/s |
Proper motion (μ) | RA: −59.68±0.65[7] mas/yr Dec.: −113.19±0.35[7] mas/yr |
Parallax (π) | 34.57 ± 0.51 mas[7] |
Distance | 94 ± 1 ly (28.9 ± 0.4 pc) |
Details | |
Mass | 1.19 + 1.13 [8] M☉ |
Luminosity | 3.47[9] L☉ |
Temperature | 6,072[10] K |
Metallicity | -0.070[10] |
Other designations | |
HD 224635: HR 9074 | |
HD 224636: HR 9075 | |
Database references | |
SIMBAD | data |
Database references | |
SIMBAD | data |
HD 224635 and HD 224636 is a pair of stars comprising a binary star system in the constellation Andromeda. They are located approximately 94 light years away[7] and they orbit each other every 717 years.[2]
The primary star is HD 224635, a magnitude 6.46[2] star (making it visible by the naked eye under very favourable conditions) with a spectral type F8[4] that is 1.19 times more massive than the Sun.[8]
The secondary star is the slightly fainter HD 224636, with an apparent visual magnitude of 6.72,[2] a spectral type G1,[4] and 1.13 times more massive than the Sun.[8]
aa546_A69_5
was invoked but never defined (see the help page).Struve1955
was invoked but never defined (see the help page).Fabricius2002
was invoked but never defined (see the help page).rv
was invoked but never defined (see the help page).vanLeeuwen2007
was invoked but never defined (see the help page).Tokovinin
was invoked but never defined (see the help page).Anderson2012
was invoked but never defined (see the help page).PASTEL
was invoked but never defined (see the help page).