HD 32453

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Right ascension05h 01m 34.5225s[2]
Declination−39° 43 04.964[2]
HD 32453
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Caelum[1]
Right ascension 05h 01m 34.5225s[2]
Declination −39° 43 04.964[2]
Apparent magnitude (V) 6.01±0.01[3]
Characteristics
Spectral type G8 III[4]
B−V color index +0.88[5]
Astrometry
Radial velocity (Rv)5.73±0.12[2] km/s
Proper motion (μ) RA: −5.456[2] mas/yr
Dec.: +32.717[2] mas/yr
Parallax (π)8.0168±0.0344 mas[2]
Distance407 ± 2 ly
(124.7 ± 0.5 pc)
Absolute magnitude (MV)+0.78[1]
Details
Mass2.40[6] M
Radius10.03[7][8] R
Luminosity50.1[9] L
Surface gravity (log g)3.18±0.14[10] cgs
Temperature5,032±61[9] K
Metallicity [Fe/H]−0.02±0.13[10] dex
Rotational velocity (v sin i)2±1.4[11] km/s
Age700[6] Myr
Other designations
CD−39°1744, HD 32453, HIP 23377, HR 1631, SAO 195501
Database references
SIMBADdata

HD 32453 (HR 1631) is a solitary star located in the southern constellation Caelum. With an apparent magnitude of 6.01,[3] 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.[2]

This star was designated Epsilon Caeli by Johann Elert Bode in his 1801 Uranographia, but this is now no longer used.[12]

HD 32453 has a classification of G8 III,[4] 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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