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HD 110458

HD 110458 ( Bayer’s designation W CEN / w Centauri) is a star in the constellation Centaurus , its apparent magnitude is +4.66 and is located about 188.4 light years from Earth .

HD 110458
Star
Observational data
( Age J2000 )
Right ascension
Declination
Distance188.4 ± 7.1 St. years (57.8 ± 2.2 pc )
Visible magnitude ( V )4.66
ConstellationCentaurus
Astrometry
Radial velocity ( R v )−12 km / s
Own movement (μ)RA: −123.27 mas per year
Dec: −30.36 mas per year
Parallax (π)17.31 ± 0.65 mas
Absolute magnitude (V)+0.85
Characteristics
Spectral classK0III
Color Index ( B - V )+1.09
Color Index ( U - B )+1.01
Variabilityabsent
physical characteristics
Weight2.7 M ☉
Radius8.5 R ☉
Temperature4950 ± 50 K
Luminosity39 L ☉
Metallicity
Other designations
HR 4831, HD 110458, CD −48 ° 7608, HIP 62012, SAO 223614, GC 17282
Database Information
SIMBAD

Features

HD 110458 - Orange giant spectral class K0, variability is absent. The mass of the star is 2.7 times that of the sun, the radius is 8.5 times that of the sun . Luminosity is 39 times more powerful than solar, the temperature is about 4950 degrees Kelvin. HD 110458 is approaching the solar system at a speed of 12 km / s.


  1. ↑ 1 2 3 4 Collaboration G. Gaia DR2 - 2018 .-- Vol. 1345.
    <a href=" https://wikidata.org/wiki/Track:Q51905050 "> </a>
  2. ↑ Park S., Kang W., Lee J. et al. Wilson-Bappu Effect: Extended to Surface Gravity // Astron. J. / J. G. III - IOP Publishing , 2013 .-- Vol. 146, Iss. 4. - P. 73. - ISSN 0004-6256 ; 1538-3881 - doi: 10.1088 / 0004-6256 / 146/4/73
    <a href=" https://wikidata.org/wiki/Track:Q2915886 "> </a> <a href=" https://wikidata.org/wiki/Track:Q669166 "> </a> <a href = " https://wikidata.org/wiki/Track:Q53997790 "> </a> <a href=" https://wikidata.org/wiki/Track:Q6234745 "> </a>
Source - https://ru.wikipedia.org/w/index.php?title=HD_110458&oldid=83926008


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