Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Aquila |
Right ascension | 19h 37m 47.31770s[1] |
Declination | −04° 38′ 51.5072″[1] |
Apparent magnitude (V) | 5.45[2] |
Characteristics | |
Spectral type | F3 IV/V[3] |
B−V color index | 0.429±0.003[2] |
Astrometry | |
Radial velocity (Rv) | −37.6±1.8[4] km/s |
Proper motion (μ) | RA: +105.381[1] mas/yr Dec.: –53.557[1] mas/yr |
Parallax (π) | 31.1671 ± 0.1422 mas[1] |
Distance | 104.6 ± 0.5 ly (32.1 ± 0.1 pc) |
Absolute magnitude (MV) | 2.98[5] |
Details | |
Mass | 1.26[6] M☉ |
Luminosity | 5.76[2] L☉ |
Surface gravity (log g) | 4.00[6] cgs |
Temperature | 6,749±80[4] K |
Metallicity [Fe/H] | 0.17[4] dex |
Rotational velocity (v sin i) | 87.0±4.4[5] km/s |
Age | 1.283[6] Gyr |
Other designations | |
Database references | |
SIMBAD | data |
42 Aquilae, abbreviated 42 Aql, is a single[8] star in the equatorial constellation of Aquila. 42 Aquilae is its Flamsteed designation. It is a dim star but visible to the naked eye under suitable viewing conditions, having an apparent visual magnitude of 5.45.[2] 42 Aql is located some 104.6 light years away, as determined from its annual parallax shift of 31.2 mas.[1] it is moving closer to the Earth with a heliocentric radial velocity of −38 km/s,[4] and is predicted to come to within 52 light-years of the Sun in around 752,000 years.[2]
The stellar classification of this star is F3 IV/V,[3] which matches an F-type star with blended spectral traits of a main sequence star and a subgiant star. It is around 1.3[6] billion years old with a relatively high rate of rotation, having a projected rotational velocity of 87 km/s.[5] The star has 1.26[6] times the mass of the Sun and is radiating 5.76[2] times the Sun's luminosity from its photosphere at an effective temperature of 6,749 K.[4] These coordinates are a source of X-ray emission, which is most likely (99.3% chance) coming from the star.[9]
GaiaDR2
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