HD 200375 Binary star system in the constellation Aquarius HD 200375 Observation data Epoch J2000      Equinox J2000 Constellation Aquarius[1] Right ascension 21h 03m 03.02378s[2] Declination +01° 31′ 55.4137″[2] Apparent magnitude (V) 6.23[3] Characteristics Spectral type F5/6V[4] U−B color index −0.01[3] B−V color index +0.47[3] Astrometry Radial velocity (Rv) 8.77±0.34[5] km/s Proper motion (μ) RA: −110.79[2] mas/yr Dec.: −53.84[2] mas/yr Parallax (π) 14.12±0.64 mas[2] Distance 230 ± 10 ly (71 ± 3 pc) Absolute magnitude (MV) 1.98[6] Details A Mass 1.53[7] M☉ Radius 2.9[8] R☉ Luminosity 13[8] L☉ Temperature 6,386[8] K B Mass 1.40[7] M☉ Temperature 5,045[9] K Other designations ADS 14573, BD+00°4648, HD 200375, HIP 103892, HR 8056, SAO 126491. A: TYC 526-1953-1 B: TYC 526-1953-2 Database references SIMBAD data A B Data sources: Hipparcos Catalogue, CCDM (2002), Bright Star Catalogue (5th rev. ed.) HD 200375 is a binary star[6] system in the equatorial constellation of Aquarius. Their orbit does not yet have a unique solution available.[10][11] References ^ 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. ^ a b c d e van Leeuwen, F. (2007). "Validation of the new Hipparcos reduction". Astronomy and Astrophysics. 474 (2): 653–664. arXiv:0708.1752. Bibcode:2007A&A...474..653V. doi:10.1051/0004-6361:20078357. S2CID 18759600. ^ a b c Mermilliod, J.-C. (1986). "Compilation of Eggen's UBV data, transformed to UBV (unpublished)". Catalogue of Eggen's UBV Data. SIMBAD. Bibcode:1986EgUBV........0M. ^ Houk, N.; Swift, C. (1999). "Michigan catalogue of two-dimensional spectral types for the HD Stars, Vol. 5". Michigan Spectral Survey. 5. Bibcode:1999MSS...C05....0H. ^ Tokovinin, A. A.; Smekhov, M. G. (January 2002). "Statistics of spectroscopic sub-systems in visual multiple stars". Astronomy and Astrophysics. 382: 118–123. Bibcode:2002A&A...382..118T. doi:10.1051/0004-6361:20011586. ^ a b Holmberg, J.; Nordström, B.; Andersen, J. (July 2009). "The Geneva-Copenhagen survey of the solar neighbourhood. III. Improved distances, ages, and kinematics". Astronomy and Astrophysics. 501 (3): 941–947. arXiv:0811.3982. Bibcode:2009A&A...501..941H. doi:10.1051/0004-6361/200811191. S2CID 118577511. ^ a b Tokovinin, Andrei (2018). "The Updated Multiple Star Catalog". The Astrophysical Journal Supplement Series. 235 (1): 6. arXiv:1712.04750. Bibcode:2018ApJS..235....6T. doi:10.3847/1538-4365/aaa1a5. ^ a b c Schofield, Mathew; Chaplin, William J.; Huber, Daniel; Campante, Tiago L.; Davies, Guy R.; Miglio, Andrea; Ball, Warrick H.; Appourchaux, Thierry; Basu, Sarbani; Bedding, Timothy R.; Christensen-Dalsgaard, Jørgen; Creevey, Orlagh; García, Rafael A.; Handberg, Rasmus; Kawaler, Steven D.; Kjeldsen, Hans; Latham, David W.; Lund, Mikkel N.; Metcalfe, Travis S.; Ricker, George R.; Serenelli, Aldo; Silva Aguirre, Victor; Stello, Dennis; Vanderspek, Roland (2019). "The Asteroseismic Target List for Solar-like Oscillators Observed in 2 minute Cadence with the Transiting Exoplanet Survey Satellite". The Astrophysical Journal Supplement Series. 241 (1): 12. arXiv:1901.10148. Bibcode:2019ApJS..241...12S. doi:10.3847/1538-4365/ab04f5. ^ Stevens, Daniel J.; Stassun, Keivan G.; Gaudi, B. Scott (2017). "Empirical Bolometric Fluxes and Angular Diameters of 1.6 Million Tycho-2 Stars and Radii of 350,000 Stars with Gaia DR1 Parallaxes". The Astronomical Journal. 154 (6): 259. arXiv:1708.05025. Bibcode:2017AJ....154..259S. doi:10.3847/1538-3881/aa957b. ^ Olevic, D.; Jovanovic, P. (2001). "New Orbital Elements for 5 Double Stars". Serbian Astronomical Journal. 164 (164): 7. Bibcode:2001SerAJ.164....7O. doi:10.2298/SAJ0164007O. ^ Malkov, O. Yu.; et al. (2012). "Dynamical Masses of a Selected Sample of Orbital Binaries". Astronomy & Astrophysics. 546: 5. Bibcode:2012A&A...546A..69M. doi:10.1051/0004-6361/201219774. A69. External links Image HD 200375 This binary or multiple star system–related article is a stub. You can help Wikipedia by expanding it. v t e

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