HD 160342

Last updated
HD 160342
V626AraLightCurve.png
A light curve for V626 Arae, plotted from Hipparcos data [1]
Observation data
Epoch J2000       Equinox J2000
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]
Distance 960 ± 20  ly
(293 ± 7  pc)
Absolute magnitude  (MV)−0.45 [7]
Details
Mass 1.1 [8]   M
Radius 95 [9]   R
Luminosity 2,002 [2]   L
Surface gravity (log g)0.48 [8]   cgs
Temperature 3,479 [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
SIMBAD data

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.

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]

Related Research Articles

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<span class="mw-page-title-main">NS Puppis</span> Star in the constellation Puppis

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<span class="mw-page-title-main">Y Centauri</span> Variable star in the constellation Centaurus

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<span class="mw-page-title-main">BQ Octantis</span> Star in the constellation Octans

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HD 39901 is an orange hued star located in the constellation Columba. It is also called HR 2069, which is the star's Bright Star Catalog designation. Eggen (1989) lists it as a member of the old disk population.

HD 1032 is a solitary star in the southern circumpolar constellation Octans. It is faintly visible to the naked eye with an apparent magnitude of 5.77 and is estimated to be 850 light years away from the Solar System based on parallax measure. However, it is receding with a heliocentric radial velocity of 4 km/s.

<span class="mw-page-title-main">AF Columbae</span> Star in the constellation of Columba

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<span class="mw-page-title-main">8 Leonis Minoris</span> Star in the constellation of Leo Minor

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<span class="mw-page-title-main">HD 168592</span> Star in the constellation of Corona Australis

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<span class="mw-page-title-main">HD 187086</span> Astrometric binary and suspected variable star

HD 187086, also known as HR 7537, is a probable astrometric binary located in the southern constellation Telescopium. It has an average apparent magnitude of 5.9, making it faintly visible to the naked eye. The star is located relatively far at a distance of 1,020 light years based on Gaia DR3 parallax measurements but is rapidly drifting closer with a heliocentric radial velocity of −64 km/s. At its current distance, HD 187086's brightness is diminished by 0.27 magnitudes due to interstellar dust. It has an absolute magnitude of −0.8.

<span class="mw-page-title-main">V718 Coronae Australis</span> Slow irregular variable; Corona Australis

V718 Coronae Australis is a solitary variable star located in the southern constellation Corona Australis. It is faintly visible to the naked eye as a red-hued point of light with an apparent magnitude of 5.43. Gaia DR3 parallax measurements imply a distance of 630 light years and it is currently receding with a heliocentric radial velocity of 28.5 km/s. At its current distance V718 CrA's brightness is diminished by 0.37 magnitudes due to interstellar dust and it has an absolute magnitude of −1.03.

<span class="mw-page-title-main">HD 192827</span> Suspected variable; Telescopium

HD 192827, also known as HR 7745 or rarely 83 G. Telescopii, is a solitary red hued star located in the southern constellation Telescopium. It has an apparent magnitude of 6.28, placing it near the limit for naked eye visibility. The object is located relatively far at a distance of 1,320 light years based on Gaia DR3 parallax measurements, but it is approaching with a heliocentric radial velocity of −43.7 km/s. At its current distance, HD 192827's brightness is diminished by 0.19 magnitudes due to interstellar dust and it has an absolute magnitude of −1.07.

<span class="mw-page-title-main">WZ Doradus</span> Semiregular variable in Dorado

WZ Doradus is a solitary red-hued variable star located in the southern constellation Dorado. It has an average apparent magnitude of 5.21, making it faintly visible to the naked eye under ideal conditions. Gaia DR3 parallax measurements imply a distance of 580 light-years and it is currently receding with a heliocentric radial velocity of 19.3 km/s. At its current distance, WZ Doradus is diminished by two-tenths of a magnitude due to interstellar extinction and it has an absolute magnitude of −1.00.

<span class="mw-page-title-main">HD 196917</span> Suspected variable star in Microscopium

HD 196917 is a solitary star located in the southern constellation Microscopium. It is faintly visible to the naked eye as a red-hued point of light with an apparent magnitude of 5.74. Gaia DR3 parallax measurements imply a distance of 426 light-years and it is rapidly approaching the Solar System with a heliocentric radial velocity of −97.3 km/s. At its current distance, HD 196917's brightness is diminished by 0.13 magnitudes due to interstellar extinction and it has an absolute magnitude of +0.04.

References

  1. "/ftp/cats/more/HIP/cdroms/cats". Centre de Données astronomiques de Strasbourg. Strasbourg astronomical Data Center. Retrieved 15 October 2022.
  2. 1 2 3 4 5 6 Vallenari, A.; et al. (Gaia collaboration) (2023). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy and Astrophysics. 674: A1. arXiv: 2208.00211 . Bibcode:2023A&A...674A...1G. doi: 10.1051/0004-6361/202243940 . S2CID   244398875. Gaia DR3 record for this source at VizieR.
  3. 1 2 3 Samus’, N. N.; Kazarovets, E. V.; Durlevich, O. V.; Kireeva, N. N.; Pastukhova, E. N. (January 2017). "General catalogue of variable stars: Version GCVS 5.1". Astronomy Reports. 61 (1): 80–88. Bibcode:2017ARep...61...80S. doi:10.1134/S1063772917010085. ISSN   1063-7729. S2CID   255195566.
  4. 1 2 Houk, Nancy (1979). Michigan catalogue of two-dimensional spectral types for the HD stars. Vol. 1. Ann Arbor, Michigan: Dept. of Astronomy, University of Michigan. Bibcode:1978mcts.book.....H.
  5. 1 2 3 "V626 Ara". SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 2022-11-23.
  6. Gontcharov, G. A. (November 2006). "Pulkovo Compilation of Radial Velocities for 35 495 Hipparcos stars in a common system". Astronomy Letters. 32 (11): 759–771. arXiv: 1606.08053 . Bibcode:2006AstL...32..759G. doi:10.1134/S1063773706110065. S2CID   119231169.
  7. Gontcharov, G. A. (2017). "VizieR Online Data Catalog: Tycho-2 red giant branch and carbon stars (Gontcharov, 2011)". VizieR On-Line Data Catalog. Bibcode:2017yCat..90370769G.
  8. 1 2 3 4 Anders, F.; et al. (August 2019). "Photo-astrometric distances, extinctions, and astrophysical parameters for Gaia DR2 stars brighter than G = 18". Astronomy & Astrophysics. 628: A94. arXiv: 1904.11302 . Bibcode:2019A&A...628A..94A. doi: 10.1051/0004-6361/201935765 . ISSN   0004-6361.
  9. Stassun, Keivan G.; et al. (9 September 2019). "The Revised TESS Input Catalog and Candidate Target List". The Astronomical Journal. 158 (4): 138. arXiv: 1905.10694 . Bibcode:2019AJ....158..138S. doi: 10.3847/1538-3881/ab3467 . eISSN   1538-3881. hdl: 1721.1/124721 . S2CID   166227927.
  10. 1 2 Eggen, Olin J. (July 1992). "Asymptotic giant branch stars near the sun". Astronomical Journal. 104 (1): 275–313. Bibcode:1992AJ....104..275E. doi:10.1086/116239.
  11. Corben, P. M. (1971). "Photoelectric Magnitudes and Colours for Bright Southern Stars". Monthly Notes of the Astron. Soc. Southern Africa. 30: 79–80. Bibcode:1971MNSSA..30...79C . Retrieved 25 November 2024.
  12. Kukarkin, B. V.; Kholopov, P. N.; Kukarkina, N. P.; Perova, N. B. (October 1973). "59th Name-List of Variable Stars". Information Bulletin on Variable Stars. 834. Bibcode:1973IBVS..834....1K . Retrieved 25 November 2024.
  13. Koen, Chris; Eyer, Laurent (March 2002). "New periodic variables from the Hipparcos epoch photometry". Monthly Notices of the Royal Astronomical Society . 331 (1): 45–59. arXiv: astro-ph/0112194 . Bibcode:2002MNRAS.331...45K. doi: 10.1046/j.1365-8711.2002.05150.x . S2CID   10505995.