HD 179433

Last updated
HD 179433
Corona Australis constellation map.svg
Red circle.svg
Location of HD 179433 (circled)
Observation data
Epoch J2000.0        Equinox J2000.0 (ICRS)
Constellation Corona Australis
Right ascension 19h 14m 39.56095s [1]
Declination −45° 11 36.6990 [1]
Apparent magnitude  (V)5.91±0.01 [2]
Characteristics
Spectral type G8 III [3]
B−V color index +0.90 [4]
Astrometry
Radial velocity (Rv)−35.1±0.4 [5]  km/s
Proper motion (μ)RA: +47.604 [1]   mas/yr
Dec.: −39.804 [1]   mas/yr
Parallax (π)9.9058 ± 0.0428  mas [1]
Distance 329 ± 1  ly
(101.0 ± 0.4  pc)
Absolute magnitude  (MV)+1.11 [6]
Details [7]
Mass 2.45±0.04  M
Radius 8.26±0.14  R
Luminosity 43.3±1.0  L
Surface gravity (log g)2.88±0.07  cgs
Temperature 5,120±30  K
Metallicity [Fe/H]−0.004±0.027  dex
Rotational velocity (v sin i)2.9±1 [8]  km/s
Age 727±10 [9]   Myr
Other designations
49 G. Coronae Australis [10] , CD−45°13054, CPD−45°9650, GC  26485, HD  179433, HIP  94556, HR  7281, SAO  229573 [11]
Database references
SIMBAD data

HD 179433, also known as HR 7281 or rarely 49 G. Coronae Australis, is a solitary star located in the southern constellation Corona Australis. It is faintly visible to the naked eye as a yellow-hued point of light with an apparent magnitude of 5.91. [2] Gaia DR3 parallax measurements imply a distance of 329 light-years, [1] and it is currently drifting closer with a heliocentric radial velocity of −35.1  km/s . [5] At its current distance, HD 179433's brightness is diminished by interstellar extinction of 0.22 magnitudes [12] and it has an absolute magnitude of +1.11. [6]

HD 179433 has a stellar classification of G8 III, [3] indicating that it is an evolved red giant. It has 2.45 times the mass of the Sun [7] but at the age of 727 million years, [9] it has expanded to 8.26 times the Sun's radius. [7] It radiates 43.3 times the luminosity of the Sun from its enlarged photosphere at an effective temperature of 5,120  K . [7] HD 197433 has a near solar metallicity at [Fe/H]= −0.0004 [7] and it spins modestly with a projected rotational velocity of 2.9  km/s . [8]

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<span class="mw-page-title-main">Iota Telescopii</span> K-type giant; Telescopium

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<span class="mw-page-title-main">2 Piscis Austrini</span> Star in the constellation Microscopium

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<span class="mw-page-title-main">HD 186302</span> Star in the constellation Pavo

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<span class="mw-page-title-main">HD 198716</span> Star in the constellation of Microscopium

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<span class="mw-page-title-main">HD 175219</span> K-type giant; Corona Australis

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<span class="mw-page-title-main">HD 101917</span> High proper motion star

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<span class="mw-page-title-main">HD 182893</span> Star in the constellation Telescopium

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<span class="mw-page-title-main">HD 189080</span> Star in the constellation of Telescopium

HD 189080, also known as HR 7621 or rarely 74 G. Telescopii, is a solitary orange-hued star located in the southern constellation Telescopium. It has an apparent magnitude of 6.18, placing it near the limit for naked eye visibility. Gaia DR3 parallax measurements place it at a distance of 357 light years and it is currently receding rapidly with a heliocentric radial velocity of 66.9 km/s. At its current distance, HD 189080's brightness is diminished by 0.17 magnitudes due to extinction from interstellar dust. It has an absolute magnitude of +1.1.

<span class="mw-page-title-main">HD 185075</span> Star in the constellation Telescopium

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References

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