HD 32453

Last updated
HD 32453
Observation data
Epoch J2000.0        Equinox J2000.0 (ICRS)
Constellation Caelum
Right ascension 05h 01m 34.5225s [1]
Declination −39° 43 04.9641 [1]
Apparent magnitude  (V)6.01±0.01 [2]
Characteristics
Spectral type G8 III [3]
B−V color index +0.88 [4]
Astrometry
Radial velocity (Rv)5.73±0.12 [1]  km/s
Proper motion (μ)RA: −5.456 [1]   mas/yr
Dec.: +32.717 [1]   mas/yr
Parallax (π)8.0168 ± 0.0344  mas [1]
Distance 407 ± 2  ly
(124.7 ± 0.5  pc)
Absolute magnitude  (MV)+0.78 [5]
Details
Mass 2.40 [6]   M
Radius 10.03 [7] [8]   R
Luminosity 50.1 [9]   L
Surface gravity (log g)3.18±0.14 [10]   cgs
Temperature 5,032±61 [9]   K
Metallicity [Fe/H]−0.02±0.13 [10]   dex
Rotational velocity (v sin i)2±1.4 [11]  km/s
Age 700 [6]   Myr
Other designations
CD–39°1744, HD  32453, HIP  23377, HR  1631, SAO  195501
Database references
SIMBAD data

HD 32453 (HR 1631) is a solitary star located in the southern constellation Caelum. With an apparent magnitude of 6.01, [2] it's barely visible to the naked eye under ideal conditions. This star is located 407 light years away based on its parallax shift, but is drifting away at a rate of 5.73 km/s. [1]

HD 32453 has a classification of G8 III, [3] which states it is an evolved G-type star that exhausted hydrogen at its core and left the main sequence. At present it has 2.40 [6] times the Sun's mass, but at an age of 700 million years, [6] HD 32453 has expanded to 10 [7] times the latter's girth (radius detected from an angular diameter of 0.748 mas [8] ). It radiates at 50 [9] solar luminosities from its enlarged photosphere at an effective temperature of 5,032 K, [9] which gives it a yellow hue. HD 32453 is slightly metal deficient, [10] and spins slowly with a projected rotational velocity of 2 km/s, [11] common for a giant star.

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References

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  7. 1 2 Lang, Kenneth R. (2006), Astrophysical formulae, Astronomy and astrophysics library, vol. 1 (3 ed.), Birkhäuser, ISBN   3-540-29692-1 . The radius (R*) is given by:
  8. 1 2 Stevens, Daniel J.; Stassun, Keivan G.; Gaudi, B. Scott (1 December 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. arXiv: 1708.05025 . Bibcode:2017AJ....154..259S. doi: 10.3847/1538-3881/aa957b . ISSN   0004-6256. S2CID   119191064.
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