Rho Telescopii

ρ Telescopii
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Telescopium
Right ascension 19h 06m 19.95580s[1]
Declination –52° 20′ 27.2757″[1]
Apparent magnitude (V) +5.17[2]
Distance185 ± 7 ly
(57 ± 2[1] pc)
Spectral typeF6 V[3]
Other designations
CP−52 11356, HD 177171, HIP 93815, HR 7213, SAO 245921.[4]

Rho Telescopii (ρ Tel, ρ Telescopii) is the Bayer designation for a star in the southern constellation of Telescopium.

Rho Telescopii is an F-type main sequence star with an apparent magnitude of around +5.17.[2] It is approximately 185 light years from Earth.[1] The mass of this star is 2.6 ± 0.1 times that of the Sun and it is around 1.5 ± 0.2 million years old. Relative to neighboring stars, it has a peculiar velocity of 17.2 km s−1.[5] It may be a member of the Tucana-Horologium association.[6]

References

  1. 1 2 3 4 van Leeuwen, Floor (November 2007), "Validation of the new Hipparcos reduction", Astronomy and Astrophysics, 474 (2): 653–664, arXiv:0708.1752v1Freely accessible, Bibcode:2007A&A...474..653V, doi:10.1051/0004-6361:20078357 Note: see VizieR catalogue I/311.
  2. 1 2 Johnson, H. L.; et al. (1966). "UBVRIJKL photometry of the bright stars". Communications of the Lunar and Planetary Laboratory. 4 (99). Bibcode:1966CoLPL...4...99J.
  3. ↑ Houk, Nancy (1978), Michigan catalogue of two-dimensional spectral types for the HD stars, 2, Ann Arbor: Dept. of Astronomy, University of Michigan, Bibcode:1978mcts.book.....H
  4. ↑ "rho Tel -- Star", SIMBAD Astronomical Object Database, Centre de Données astronomiques de Strasbourg, retrieved 2012-03-28
  5. ↑ Tetzlaff, N.; Neuhäuser, R.; Hohle, M. M. (January 2011), "A catalogue of young runaway Hipparcos stars within 3 kpc from the Sun", Monthly Notices of the Royal Astronomical Society, 410 (1): 190–200, arXiv:1007.4883Freely accessible, Bibcode:2011MNRAS.410..190T, doi:10.1111/j.1365-2966.2010.17434.x
  6. ↑ Fernández, D.; Figueras, F.; Torra, J. (March 2008), "On the kinematic evolution of young local associations and the Scorpius-Centaurus complex", Astronomy and Astrophysics, 480 (3): 735–751, arXiv:0801.0605Freely accessible, Bibcode:2008A&A...480..735F, doi:10.1051/0004-6361:20077720


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