HD 88522
Observation data
Epoch J2000      Equinox J2000
Constellation Antlia
Right ascension 10h 12m 02.85179s[1]
Declination −28° 36′ 21.4485″[1]
Apparent magnitude (V) 6.28 (6.78 + 7.41)[2]
Characteristics
Spectral type A1 V (A1 V + A2 V)[2]
B−V color index 0.019±0.004[3]
Astrometry
Radial velocity (Rv)+27.4±0.4[4] km/s
Proper motion (μ) RA: −38.74[1] mas/yr
Dec.: −1.24[1] mas/yr
Parallax (π)6.55 ± 0.58 mas[1]
Distance500 ± 40 ly
(150 ± 10 pc)
Absolute magnitude (MV)0.86 + 1.49[2]
Orbit[5]
Period (P)91.89±0.85 yr
Semi-major axis (a)0.226±0.003″
Eccentricity (e)0.676±0.012
Inclination (i)76.0±0.7°
Longitude of the node (Ω)198.3±0.5°
Periastron epoch (T)2003.58±0.22
Argument of periastron (ω)
(secondary)		59.7±1.1°
Details
HD 88522 A
Mass2.53[2] M☉
Luminosity75.8+16.6
−13.6[6] L☉
Temperature9,638+134
−132[6] K
Rotational velocity (v sin i)24[6] km/s
HD 88522 B
Mass2.17[2] M☉
Other designations
CD−27° 7266, HD 88522, HIP 49967, HR 4003, SAO 178526, WDS J10120-2836AB[7]
Database references
SIMBADdata

HD 88522 is a double or multiple star. The component stars are two white stars of similar spectral type—A1V and A2V—and luminosity.[2]

References

  1. 1 2 3 4 5 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.
  2. 1 2 3 4 5 6 Cvetkovic, Z.; Ninkovic, S. (2010), "On the Component Masses of Visual Binaries", Serbian Astronomical Journal, 180 (180): 71–80, Bibcode:2010SerAJ.180...71C, doi:10.2298/SAJ1080071C. Values from Method II listed.
  3. ↑ 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.
  4. ↑ de Bruijne, J. H. J.; Eilers, A.-C. (October 2012), "Radial velocities for the HIPPARCOS-Gaia Hundred-Thousand-Proper-Motion project", Astronomy & Astrophysics, 546: 14, arXiv:1208.3048, Bibcode:2012A&A...546A..61D, doi:10.1051/0004-6361/201219219, S2CID 59451347, A61.
  5. ↑ Tokovinin, Andrei; et al. (August 2015), "Speckle Interferometry at SOAR in 2014", The Astronomical Journal, 150 (2): 17, arXiv:1506.05718, Bibcode:2015AJ....150...50T, doi:10.1088/0004-6256/150/2/50, S2CID 30737411, 50.
  6. 1 2 3 Zorec, J.; Royer, F. (January 2012), "Rotational velocities of A-type stars. IV. Evolution of rotational velocities", Astronomy & Astrophysics, 537: A120, arXiv:1201.2052, Bibcode:2012A&A...537A.120Z, doi:10.1051/0004-6361/201117691, S2CID 55586789.
  7. ↑ "HD 88522". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2018-05-08.
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