Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Aquila |
Right ascension | 18h 56m 22.660s[1] |
Declination | −01° 47′ 59.50″[1] |
Apparent magnitude (V) | 6.20[2] |
Characteristics | |
Spectral type | B9 IIIp(HgMnEu st, CaMg wk)[3] B9 V[4] |
B−V color index | −0.046±0.005[2] |
Variable type | Stable[4] |
Astrometry | |
Radial velocity (Rv) | −26±4[2] km/s |
Proper motion (μ) | RA: −2.811 mas/yr Dec.: −19.318 mas/yr |
Parallax (π) | 6.3201 ± 0.0448 mas[1] |
Distance | 516 ± 4 ly (158 ± 1 pc) |
Absolute magnitude (MV) | 0.22[2] |
Details | |
Mass | 3.12±0.1[4] M☉ |
Radius | 2.66±0.28[4] R☉ |
Luminosity | 94.56[2] L☉ |
Surface gravity (log g) | 4.03[5] cgs |
Temperature | 12324±9[5] K |
Metallicity [Fe/H] | 0.18±0.04[2] dex |
Rotational velocity (v sin i) | 1.6±0.3[6] km/s |
Other designations | |
Database references | |
SIMBAD | data |
HD 175640 is a star in the equatorial constellation of Aquila. It has an apparent visual magnitude of 6.20,[2] which is bright enough to be visible to the naked eye under suitable seeing conditions. The star is located at a distance of approximately 516 light years as determined through parallax measurements.[1] At that distance, the star's color is modified by an extinction of 0.36 magnitude due to interstellar dust.[8] It is drifting closer with a heliocentric radial velocity of roughly −26 km/s.[2]
This is classified as a mercury-manganese star, which is a late B-type chemically peculiar star of type CP3. A distinctive feature of this class of stars is an apparent extreme overabundance of the elements mercury and manganese.[9] It has a low longitudinal magnetic field strength of −0.6±2.2 G.[6] This is a particularly stable star, showing no signs of pulsation.[4] As with other HgMn stars, it is spinning slowly, showing a projected rotational velocity of 1.6 km/s.[6]
In 2007, some evidence was found that this may be a single-lined spectroscopic binary star system. In particular, shifts in radial velocity were observed in the range of 7 to −7 km/s.[10]
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