Astronomy:HD 200375

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Short description: Binary star system in the constellation Aquarius
HD 200375
Observation data
Equinox J2000.0]] (ICRS)
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[2] mas
Distance230 ± 10 ly
(71 ± 3 pc)
Absolute magnitude (MV)1.98[6]
Orbit[7]
Period (P)840±380 yr
Semi-major axis (a)1.84±0.42″
Eccentricity (e)0.45±0.13
Inclination (i)133±7°
Longitude of the node (Ω)105±17°
Periastron epoch (T)2076±15
Argument of periastron (ω)
(secondary)		59±20°
Details
A
Mass1.53[8] M☉
Radius2.9[9] R☉
Luminosity13[9] L☉
Temperature6,386[9] K
B
Mass1.40[8] M☉
Temperature5,045[10] 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
SIMBADdata
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.

References

  1. ↑ Anderson, E.; Francis, Ch. (2012). "XHIP: An extended hipparcos compilation". Astronomy Letters 38 (5): 331. doi:10.1134/S1063773712050015. Bibcode: 2012AstL...38..331A. 
  2. ↑ 2.0 2.1 2.2 2.3 2.4 van Leeuwen, F. (2007). "Validation of the new Hipparcos reduction". Astronomy and Astrophysics 474 (2): 653–664. doi:10.1051/0004-6361:20078357. Bibcode: 2007A&A...474..653V. 
  3. ↑ 3.0 3.1 3.2 Mermilliod, J.-C. (1986). "Compilation of Eggen's UBV data, transformed to UBV (unpublished)". Catalogue of Eggen's UBV Data. SIMBAD. Bibcode: 1986EgUBV........0M. 
  4. ↑ 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. 
  5. ↑ Tokovinin, A. A.; Smekhov, M. G. (January 2002). "Statistics of spectroscopic sub-systems in visual multiple stars". Astronomy and Astrophysics 382: 118–123. doi:10.1051/0004-6361:20011586. Bibcode: 2002A&A...382..118T. 
  6. ↑ 6.0 6.1 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. doi:10.1051/0004-6361/200811191. Bibcode: 2009A&A...501..941H. 
  7. ↑ Izmailov, Igor; Khovritchev, Maxim (January 2025). "New Orbital Parameters of 850 Wide Visual Binary Stars and Their Statistical Properties" (in en). Research in Astronomy and Astrophysics 25 (1): 015016. doi:10.1088/1674-4527/ad9da3. ISSN 1674-4527. Bibcode: 2025RAA....25a5016I. 
  8. ↑ 8.0 8.1 Tokovinin, Andrei (2018). "The Updated Multiple Star Catalog". The Astrophysical Journal Supplement Series 235 (1): 6. doi:10.3847/1538-4365/aaa1a5. Bibcode: 2018ApJS..235....6T. 
  9. ↑ 9.0 9.1 9.2 Schofield, Mathew; Chaplin, William J.; Huber, Daniel; Campante, Tiago L.; Davies, Guy R.; Miglio, Andrea; Ball, Warrick H.; Appourchaux, Thierry et al. (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. doi:10.3847/1538-4365/ab04f5. Bibcode: 2019ApJS..241...12S. 
  10. ↑ 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. doi:10.3847/1538-3881/aa957b. Bibcode: 2017AJ....154..259S. 




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