56 Aquilae (original) (raw)
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K-type giant star in the constellation Aquila
56 Aquilae
| Observation dataEpoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Aquila |
| Right ascension | 19h 54m 08.27613s[1] |
| Declination | –08° 34′ 27.1674″[1] |
| Apparent magnitude (V) | 5.79[2] |
| Characteristics | |
| Spectral type | K5 III[3] |
| U−B color index | +2.00[2] |
| B−V color index | +1.664±0.006[4] |
| Astrometry | |
| Radial velocity (Rv) | −49.5±2.9[5] km/s |
| Proper motion (μ) | RA: +6.737[1] mas/yr Dec.: –18.578[1] mas/yr |
| Parallax (π) | 5.6650 ± 0.1739 mas[1] |
| Distance | 580 ± 20 ly (177 ± 5 pc) |
| Absolute magnitude (MV) | −0.66[4] |
| Details | |
| Radius | 41.7+2.0−2.6[1] R☉ |
| Luminosity | 391±14[1] L☉ |
| Temperature | 3,972+130−91[1] K |
| Other designations | |
| 56 Aql, BD–08°5150, FK5 2131, GC 2343, HD 188154, HIP 97928, HR 7584, SAO 143894[6] | |
| Database references | |
| SIMBAD | data |
56 Aquilae is a single[7] star in the equatorial constellation of Aquila. 56 Aquilae is its Flamsteed designation. Its apparent visual magnitude is 5.79,[2] meaning it is barely visible to the naked eye as a dim, orange-hued point of light, under ideal viewing conditions. The star is located at a distance of around 580 light years away from the Sun, based on parallax.[1] It is moving closer to the Earth with a heliocentric radial velocity of −50 km/s,[5] and is predicted to come as near as 222 light-years in around 3.3 million years.
This is an aging giant star with a stellar classification of K5 III,[3] having exhausted the supply of hydrogen at its core and expanded to 42[1] times the Sun's radius. It is radiating 391[1] times the luminosity of the Sun from its photosphere at an effective temperature of 3,972 K.[1] 56 Aquilae is a double star,[8] but it does not appear to be a binary star system.[7] It is one of the double stars profiled in Admiral William Henry Smyth's 1864 work, Sidereal Chromatics.
- ^ a b c d e f g h i j k l Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv:1804.09365. Bibcode:2018A&A...616A...1G. doi:10.1051/0004-6361/201833051. Gaia DR2 record for this source at VizieR.
- ^ a b c Nicolet, B. (1978), "Photoelectric photometric Catalogue of homogeneous measurements in the UBV System", Astronomy and Astrophysics Supplement Series, 34: 1–49, Bibcode:1978A&AS...34....1N.
- ^ a b Houk, N.; Swift, C. (1999), "Michigan catalogue of two-dimensional spectral types for the HD Stars", Michigan Spectral Survey, 5, Bibcode:1999MSS...C05....0H.
- ^ a b Anderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation", Astronomy Letters, 38 (5): 331, arXiv:1108.4971, Bibcode:2012AstL...38..331A, doi:10.1134/S1063773712050015, S2CID 119257644.
- ^ a b Wilson, Ralph Elmer (1953), "General Catalogue of Stellar Radial Velocities", Carnegie Institute Washington D.C. Publication, Washington: Carnegie Institution of Washington, Bibcode:1953GCRV..C......0W.
- ^ "56 Aql". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2019-08-01.
- ^ a b Eggleton, P. P.; Tokovinin, A. A. (September 2008), "A catalogue of multiplicity among bright stellar systems", Monthly Notices of the Royal Astronomical Society, 389 (2): 869–879, arXiv:0806.2878, Bibcode:2008MNRAS.389..869E, doi:10.1111/j.1365-2966.2008.13596.x, S2CID 14878976.
- ^ James, Andrew, The application of Admiral Smyth's "Sidereal Chromatics", archived from the original on 2009-10-26, retrieved 2007-12-22.