HD 202951

HD 202951 is a probable binary star system located in the northern constellation of Equuleus. It is near the lower limit of visibility to the naked eye, having an apparent visual magnitude of 5.97.[2] The distance to this system can be estimated from the annual parallax shift of 2.74 mas,[1] yielding a value of roughly 1,190 light years. It is moving closer with a heliocentric radial velocity of −37 km/s.[4]

HD 202951
Observation data
Epoch J2000      Equinox J2000
Constellation Equuleus
Right ascension 21h 18m 52.02476s[1]
Declination +11° 12 12.1752[1]
Apparent magnitude (V) 5.97[2]
Characteristics
Spectral type K5 III[2]
B−V color index 1.648[3]
Astrometry
Radial velocity (Rv)−37.3±2.5[4] km/s
Proper motion (μ) RA: +23.728 mas/yr
Dec.: +15.448 mas/yr
Parallax (π)2.7415 ± 0.1321[1] mas
Distance1,190 ± 60 ly
(360 ± 20 pc)
Absolute magnitude (MV)−1.97[3]
Orbit[5]
Period (P)999.8±2.4 d
Eccentricity (e)0.229±0.018
Periastron epoch (T)53771 ± 12 MJD
Argument of periastron (ω)
(secondary)
3±5°
Semi-amplitude (K1)
(primary)
4.09±0.08 km/s
Details
Luminosity5.15[2] L
Rotational velocity (v sin i)4.4[6] km/s
Other designations
NSV 25543, BD+10° 4516, FK5 3700, HD 202951, HIP 105224, HR 8149, SAO 107020[7]
Database references
SIMBADdata

Griffin (2012) found this to be a single-lined spectroscopic binary system with an orbital period of 2.7373 ± 0.0066 yr and an eccentricity of 0.23. The a sin i value for the primary component is 54.8 ± 1.1 Gm (0.366 ± 0.007 AU), where a is the semimajor axis and i is the (unknown) orbital inclination. This value provides a lower bound for the actual semimajor axis.[5]

The visible component is an evolved K-type giant star with a stellar classification of K5 III.[2] It is a candidate variable star of unknown type, showing an amplitude variation of 0.0115 magnitude with a frequency of 0.47645 times per day, or one cycle per 2.1 days.[8] X-ray emission has been detected from this system.[9]

References

  1. 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.
  2. 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.
  3. Ryon, Jenna; et al. (August 2009), "Comparing the Ca ii H and K Emission Lines in Red Giant Stars", Publications of the Astronomical Society of the Pacific, 121 (882): 842, arXiv:0907.3346, Bibcode:2009PASP..121..842R, doi:10.1086/605456.
  4. Gontcharov, G. A. (2006), "Pulkovo Compilation of Radial Velocities for 35 495 Hipparcos stars in a common system", Astronomy Letters, 32 (11): 759–771, arXiv:1606.08053, Bibcode:2006AstL...32..759G, doi:10.1134/S1063773706110065.
  5. Griffin, R. F. (February 2012), "Spectroscopic binary orbits from photoelectric radial velocities - Paper 222: HR 4241, HR 7208, HR 8026, and HR 8149", The Observatory, 132 (1): 16–33, Bibcode:2012Obs...132...16G.
  6. De Medeiros, J. R.; et al. (October 2002), "The Rotation of Binary Systems with Evolved Components", The Astrophysical Journal, 578 (2): 943–950, arXiv:astro-ph/0207288, Bibcode:2002ApJ...578..943D, doi:10.1086/342613.
  7. "HD 202951". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2018-07-20.
  8. Koen, Chris; Eyer, Laurent (2002), "New periodic variables from the Hipparcos epoch photometry", Monthly Notices of the Royal Astronomical Society, 331: 45, arXiv:astro-ph/0112194, Bibcode:2002MNRAS.331...45K, doi:10.1046/j.1365-8711.2002.05150.x.
  9. Smith, Graeme H.; Shetrone, Matthew D. (2000), "CaII K Emission-Line Asymmetry among Red Giants Detected by the ROSAT Satellite", The Publications of the Astronomical Society of the Pacific, 112 (776): 1320, Bibcode:2000PASP..112.1320S, doi:10.1086/316634.
This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.