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HD 160342

Star in the constellation Ara From Wikipedia, the free encyclopedia

HD 160342 is a star in the southern constellation of Ara. HD 160342 is its Henry Draper Catalogue designation. It has an apparent visual magnitude of 6.35,[10] making it very faintly visible to the naked eye under ideal observing conditions. Based upon parallax measurements, is approximately 960 light-years (293 parsecs) distant from Earth.

Right ascension17h 42m 03.62014s[2]
Declination−50° 30 38.5331[2]
Apparentmagnitude(V)6.23 - 6.46[3]
Quick facts Constellation, Right ascension ...
HD 160342

A light curve for V626 Arae, plotted from Hipparcos data[1]
Observation data
Epoch J2000      Equinox ICRS
Constellation Ara
Right ascension 17h 42m 03.62014s[2]
Declination −50° 30 38.5331[2]
Apparent magnitude (V) 6.23 - 6.46[3]
Characteristics
Spectral type M3 III[4]
U−B color index +1.96[5]
B−V color index +1.73[5]
R−I color index 0.85
Variable type LB[3]
Astrometry
Radial velocity (Rv)−27.1±0.4[6] km/s
Proper motion (μ) RA: +3.096[2] mas/yr
Dec.: −15.788[2] mas/yr
Parallax (π)3.4132±0.0864 mas[2]
Distance960 ± 20 ly
(293 ± 7 pc)
Absolute magnitude (MV)−0.45[7]
Details
Mass1.1[8] M
Radius95[9] R
Luminosity2,002[2] L
Surface gravity (log g)0.48[8] cgs
Temperature3,479[8] K
Metallicity [Fe/H]−0.05[8] dex
Other designations
CD−50°11474, HD 160342, HIP 86628, HR 6576, SAO 244954, V626 Arae.[5]
Database references
SIMBADdata
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In 1971, P. M. Corben announced that HD 160342 is a variable star, a discovery made using a telescope equipped with a photoelectric photometer at the Royal Observatory in South Africa.[11] It was given its variable star designation, V626 Arae, in 1973.[12]

With a stellar classification of M3 III,[4] this is an evolved red giant that is on the asymptotic giant branch.[10] It is a variable star that is classified as irregular,[3] although changes in brightness of 0.1127 magnitudes at the rate of 0.37943 cycles per day (once every 2.6 days) have been detected in Hipparcos photometry.[13]

References

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