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HD 19789

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HD 19789
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Aries[1]
Right ascension 03h 11m 21.91898s[2]
Declination +13° 02′ 52.2342″[2]
Apparent magnitude (V) 6.11[1]
Characteristics
Evolutionary stage red giant branch[2]
Spectral type K0IIIp[3]
B−V color index 1.038±0.012[1]
Astrometry
Radial velocity (Rv)+8.10±0.32[1] km/s
Proper motion (μ) RA: −15.387[2] mas/yr
Dec.: +16.445[2] mas/yr
Parallax (π)8.4809±0.0283 mas[2]
Distance385 ± 1 ly
(117.9 ± 0.4 pc)
Absolute magnitude (MV)0.53[1]
Details
Mass2.6[2] M
Radius11[2] R
Luminosity63[2] L
Surface gravity (log g)2.67[2] cgs
Temperature4.933[2] K
Age558[2] Myr
Other designations
BD+12°452, FK5 2488, HD 19789, HIP 14821, HR 952, SAO 93327, WDS WDS J03114+1303AB[4]
Database references
SIMBADdata

HD 19789 is a double star in the northern constellation of Aries. The primary component has an orange hue and is barely visible to the naked eye with an apparent visual magnitude of 6.11.[1] it is located at a distance of approximately 385 light years from the Sun based on parallax,[2] and is drifting further away with a radial velocity of +8 km/s.[1] The star is located near the ecliptic and thus is subject to lunar occultations.[5]

The primary, designated component A, is an aging giant star with a stellar classification of K0IIIp,[3] where the 'p' suffix indicates some type of unspecified peculiarity in the spectrum. It has exhausted the supply of hydrogen at its core, then expanded and cooled off the main sequence: at present it has 11 times the girth of the Sun. The star is radiating 63 times the Sun's luminosity from its swollen photosphere at an effective temperature of 4,933 K.[2] It has one reported companion, component B, at an angular separation of 0.5 along a position angle of 23°, as of 1982.[6]

References

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  1. ^ a b c d e f g 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. XHIP record for this object at VizieR.
  2. ^ a b c d e f g h i j k l m n Vallenari, A.; et al. (Gaia collaboration) (2023). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy and Astrophysics. 674: A1. arXiv:2208.00211. Bibcode:2023A&A...674A...1G. doi:10.1051/0004-6361/202243940. S2CID 244398875. Gaia DR3 record for this source at VizieR.
  3. ^ a b Harlan, E. A. (September 1969), "MK classifications for F- and G-type stars. I", Astronomical Journal, 74: 916–919, Bibcode:1969AJ.....74..916H, doi:10.1086/110881.
  4. ^ "HD 19789". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2011-12-20.
  5. ^ Blow, G. L.; et al. (November 1982), "Photoelectric observations of lunar occultations. XIII", Astronomical Journal, 87: 1571–1584, Bibcode:1982AJ.....87.1571B, doi:10.1086/113247. See entry 5931, p. 1580, SAO 93327.
  6. ^ Mason, B. D.; et al. (2014), "The Washington Visual Double Star Catalog", The Astronomical Journal, 122 (6): 3466, Bibcode:2001AJ....122.3466M, doi:10.1086/323920, retrieved 2015-07-22