Observation data Epoch J2000.0 (ICRS) Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Aquarius |
Right ascension | 23h 41m 34.48893s[1] |
Declination | −18° 01′ 37.4656″[1] |
Apparent magnitude (V) | 5.34[2] |
Characteristics | |
Spectral type | K4/K5 III[3] |
B−V color index | +1.57[2] |
Astrometry | |
Radial velocity (Rv) | +25.1[4] km/s |
Proper motion (μ) | RA: –41.665[1] mas/yr Dec.: –71.428[1] mas/yr |
Parallax (π) | 4.6918 ± 0.2010 mas[1] |
Distance | 700 ± 30 ly (213 ± 9 pc) |
Details | |
Radius | 63.58+0.54 −0.99[1] R☉ |
Luminosity | 848.285±41.525[1] L☉ |
Surface gravity (log g) | 1.59[5] cgs |
Temperature | 3,910[5] K |
Metallicity [Fe/H] | –0.18[5] dex |
Other designations | |
Database references | |
SIMBAD | data |
103 Aquarii is a single[7] star in the equatorial constellation of Aquarius. 103 Aquarii is the Flamsteed designation, although it also bears the Bayer designation A1 Aquarii.[8] It is faint but visible to the naked eye as an orange hued star with an apparent visual magnitude of 5.34.[2] Based upon an annual parallax shift of 4.69 mas, the distance to this star is around 700 light-years (210 parsecs).[1] It is moving away from the Earth with a heliocentric radial velocity of +25 km/s.[4]
This is classified as a K-type giant star,[3] having evolved off the main sequence after exhausting the hydrogen at its core and expanded to 64[1] times the Sun's radius. The star is radiating 848[1] times the luminosity of the Sun from its enlarged photosphere at an effective temperature of 3,910 K.[5]
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