HD 171978 is a binary star system in the Serpens Cauda segment of the equatorial constellation of Serpens. It may be referred to by its Bright Star Catalogue identifier of HR 6993. This system is dimly visible to the naked eye with a combined apparent visual magnitude of 5.76,[6] although is a suspected variable star of unknown type with a magnitude that has been reported to vary between 5.74 and 5.86.[3] HD 171978 is located at a distance of approximately 537 light-years from the Sun based on parallax,[1] and is drifting further away with a barycentric radial velocity of +11.4 km/s.[2] It is a member of the Ursa Major Moving Group.[8]
| Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
|---|---|
| Constellation | Serpens |
| Right ascension | 18h 37m 35.9626s[1] |
| Declination | −00° 18′ 34.100″[1] |
| Apparent magnitude (V) | 6.33±0.10 (A)[2] 6.73±0.10 (B)[2] 5.74 to 5.86 (AB)[3] |
| Characteristics | |
| Spectral type | A0V[4] |
| U−B color index | +0.06[5] |
| B−V color index | +0.067±0.010[6] |
| R−I color index | +0.04[5] |
| Variable type | suspected[3] |
| Astrometry | |
| Radial velocity (Rv) | +11.415±0.031[2] km/s |
| Proper motion (μ) | RA: +14.018[1] mas/yr Dec.: −20.710[1] mas/yr |
| Parallax (π) | 6.0774 ± 0.0833 mas[1] |
| Distance | 537 ± 7 ly (165 ± 2 pc) |
| Absolute magnitude (MV) | 0.30±0.15 (A)[2] 0.70±0.15 (B)[2] |
| Orbit[2] | |
| Period (P) | 14.684636±0.000029 d |
| Eccentricity (e) | 0.2495±0.0011 |
| Periastron epoch (T) | 2,454,405.073±0.011 |
| Argument of periastron (ω) (secondary) | 230.90±0.30° |
| Semi-amplitude (K1) (primary) | 37.918±0.050 km/s |
| Semi-amplitude (K2) (secondary) | 38.569±0.076 km/s |
| Details[2] | |
| A | |
| Mass | 2.5 M☉ |
| Radius | 3.4±0.3 R☉ |
| Luminosity | 60.5±8.5 L☉ |
| Rotational velocity (v sin i) | 5.6±1.0 km/s |
| B | |
| Mass | 2.35 M☉ |
| Radius | 2.8±0.2 R☉ |
| Luminosity | 41.9±5.9 L☉ |
| Rotational velocity (v sin i) | 5.9±1.0 km/s |
| Other designations | |
| Database references | |
| SIMBAD | data |
The binary nature of this system was reported by Canadian astronomer R. M. Petrie in 1948.[9] It is a double-lined spectroscopic binary with an orbital period of 14.7 days and an eccentricity (ovalness) of 0.25. The orbital inclination is estimated to be ~30°. The two stars have a magnitude difference of 0.4±0.1 mag, which gives respective magnitudes of 6.33 and 6.73. They each show a sharp-lined spectra, indicating their rotation rates are not high. Both are similar A-type main-sequence stars[2] with a combined stellar classification of A0V.[4] In 1970, Geary and Abt noted that the secondary appeared to be an Am star.[8]
References
edit- ^ a b c d e f 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 d e f g h i Fekel, Francis C.; Tomkin, Jocelyn; Williamson, Michael H. (2013). "New Precision Orbits of Bright Double-lined Spectroscopic Binaries. VIII. HR 1528, HR 6993, 2 Sagittae, and 18 Vulpeculae". The Astronomical Journal. 146 (5). 129. Bibcode:2013AJ....146..129F. doi:10.1088/0004-6256/146/5/129. hdl:2152/34407. S2CID 121155872.
- ^ a b c "NSV 11122, database entry". New Catalogue of Suspected Variable Stars, the improved version. Moscow, Russia: Sternberg Astronomical Institute. Retrieved October 3, 2008.
- ^ 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 Hoffleit, D.; Warren, Jr., W. H. HR 6993, database entry (5th Revised ed.). Centre de Données astronomiques de Strasbourg. Retrieved October 3, 2008.
{{cite book}}:|work=ignored (help) V/50. - ^ 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.
- ^ "e Ser". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2015-12-07.
- ^ a b Geary, J. C.; Abt, H. A. (August 1970). "Rotational velocities in the Ursa Major group". Astronomical Journal. 75: 718–720. Bibcode:1970AJ.....75..718G. doi:10.1086/111013.
- ^ Petrie, R. M. (July 1948). "The spectrographic orbits and dimensions of H. D. 171978". Publications of the Dominion Astrophysical Observatory Victoria. 7: 415–418. Bibcode:1948PDAO....7..415P.