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Kappa Telescopii

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Star in the constellation Telescopium
Kappa Telescopii
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Telescopium
Right ascension 18 52 39.64405
Declination −52° 06′ 26.5372″
Apparent magnitude (V) +5.20
Characteristics
Spectral type G8/K0 III
B−V color index +0.96
Astrometry
Radial velocity (Rv)−44.3 km/s
Proper motion (μ) RA: +39.92 mas/yr
Dec.: −96.17 mas/yr
Parallax (π)12.00 ± 0.27 mas
Distance272 ± 6 ly
(83 ± 2 pc)
Absolute magnitude (MV)+0.41±0.14
Details
Mass1.92 M
Radius10.51 R
Luminosity77.6 L
Surface gravity (log g)2.79 cgs
Temperature4,968 K
Metallicity −0.25 dex
Rotational velocity (v sin i)2.63 km/s
Age1.25 Gyr
Other designations
κ Tel, CPD−52° 11268, FK5 3499, HD 174295, HIP 92646, HR 7087, SAO 245772
Database references
SIMBADdata

Kappa Telescopii (κ Telescopii) is a solitary, yellow-hued star in the southern constellation of Telescopium. With an apparent visual magnitude of +5.20, it is visible to the naked eye. Based upon an annual parallax shift of 12.00 mas as seen from Earth, it is located around 272 light years from the Sun.

At the age of around 1.25 billion years, this an evolved giant star with a stellar classification of G8/K0 III, showing a spectrum with characteristics intermediate between a G-type and a K-type star. It has an estimated 1.9 times the mass of the Sun and 10.5 times the Sun's radius. The star is radiating 77.6 times the solar luminosity from its photosphere at an effective temperature of 4,968 K. It is unclear whether it is cooling or heating up on its evolutionary pathway through the red clump.

References

  1. ^ van Leeuwen, F. (2007), "Validation of the new Hipparcos reduction", Astronomy and Astrophysics, 474 (2): 653–664, arXiv:0708.1752, Bibcode:2007A&A...474..653V, doi:10.1051/0004-6361:20078357, S2CID 18759600.
  2. ^ Corben, P. M.; Stoy, R. H. (1968), "Photoelectric Magnitudes and Colours for Bright Southern Stars", Monthly Notes of the Astronomical Society of Southern Africa, 27: 11, Bibcode:1968MNSSA..27...11C.
  3. ^ Houk, Nancy; Cowley, A. P. (1978), Michigan catalogue of two-dimensional spectral types for the HD stars, vol. 1, Ann Arbor: Dept. of Astronomy, University of Michigan, Bibcode:1975mcts.book.....H.
  4. Wielen, R.; et al. (1999), "Sixth Catalogue of Fundamental Stars (FK6). Part I. Basic fundamental stars with direct solutions", Veroeffentlichungen des Astronomischen Rechen-Instituts Heidelberg, 35 (35), Astronomisches Rechen-Institut Heidelberg: 1, Bibcode:1999VeARI..35....1W.
  5. ^ da Silva, L.; et al. (November 2006), "Basic physical parameters of a selected sample of evolved stars", Astronomy and Astrophysics, 458 (2): 609–623, arXiv:astro-ph/0608160, Bibcode:2006A&A...458..609D, doi:10.1051/0004-6361:20065105, S2CID 9341088.
  6. ^ Jofré, E.; et al. (2015), "Stellar parameters and chemical abundances of 223 evolved stars with and without planets", Astronomy & Astrophysics, 574: A50, arXiv:1410.6422, Bibcode:2015A&A...574A..50J, doi:10.1051/0004-6361/201424474, S2CID 53666931.
  7. "kap Tel". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2017-06-05.{{cite web}}: CS1 maint: postscript (link)
  8. Eggleton, P. P.; Tokovinin, A. A. (September 2008), "A catalogue of multiplicity among bright stellar systems", Monthly Notices of the Royal Astronomical Society, 389 (2): 869–879, arXiv:0806.2878, Bibcode:2008MNRAS.389..869E, doi:10.1111/j.1365-2966.2008.13596.x, S2CID 14878976.
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