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2 Sextantis

From Wikipedia, the free encyclopedia
2 Sextantis
Location of 2 Sextantis (circled in red)
Observation data
Epoch J2000.0      Equinox ICRS
Constellation Hydra[1]
Right ascension 09h 38m 27.28962s[2]
Declination +04° 38 57.4461[2]
Apparent magnitude (V) 4.68[3]
Characteristics
Evolutionary stage giant
Spectral type K3 III[3]
B−V color index +1.310±0.033[1]
Astrometry
Radial velocity (Rv)+44.61±0.23[4] km/s
Proper motion (μ) RA: −163.18[2] mas/yr
Dec.: −50.88[2] mas/yr
Parallax (π)11.04±0.27 mas[2]
Distance295 ± 7 ly
(91 ± 2 pc)
Absolute magnitude (MV)−0.10[1]
Details
Mass1.32[3] M
Radius24[4] R
Luminosity191[3] L
Surface gravity (log g)2.09±0.22[5] cgs
Temperature4,188±33[3] K
Metallicity [Fe/H]−0.30±0.09[5] dex
Rotational velocity (v sin i)3.0[4] km/s
Age4.58[3] Gyr
Other designations
2 Sex, BD+05°2207, FK5 1249, HD 83425, HIP 47310, HR 3834, SAO 117821[6]
Database references
SIMBADdata

2 Sextantis is a single[7] star that is now in the equatorial constellation Hydra with the Bayer designation H Hydrae.[8] It is located around 295 light-years away from the Sun and it is visible to the naked eye as a faint, orange-hued star with an apparent visual magnitude of 4.68.[3] This object is moving further from the Earth with a heliocentric radial velocity of +44.6 km/s.[4] It has a relatively high proper motion, traversing the celestial sphere at the rate of 0.173 per year.[9]

This is a giant star with a stellar classification of K3 III,[3] which, at the age of 4.58[3] billion years old, has exhausted the hydrogen at its core and evolved away from the main sequence. The star has 1.32 times the mass of the Sun[3] and has expanded to 24 times the Sun's radius.[4] It is radiating 191 times the luminosity of the Sun from its enlarged photosphere at an effective temperature of 4,188 K.[3]

References

[edit]
  1. 1 2 3 Anderson, E.; Francis, Ch. (2012). "XHIP: An extended hipparcos compilation". Astronomy Letters. 38 (5): 331. arXiv:1108.4971. Bibcode:2012AstL...38..331A. doi:10.1134/S1063773712050015. XHIP record for this object at VizieR.
  2. 1 2 3 4 5 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.
  3. 1 2 3 4 5 6 7 8 9 10 11 Luck, R. Earle (2015), "Abundances in the Local Region. I. G and K Giants", The Astronomical Journal, 150 (3): 88, arXiv:1507.01466, Bibcode:2015AJ....150...88L, doi:10.1088/0004-6256/150/3/88, S2CID 118505114.
  4. 1 2 3 4 5 Massarotti, Alessandro; et al. (January 2008), "Rotational and Radial Velocities for a Sample of 761 Hipparcos Giants and the Role of Binarity", The Astronomical Journal, 135 (1): 209–231, Bibcode:2008AJ....135..209M, doi:10.1088/0004-6256/135/1/209.
  5. 1 2 Prugniel, Ph.; et al. (July 2011), "The atmospheric parameters and spectral interpolator for the MILES stars", Astronomy & Astrophysics, 531: A165, arXiv:1104.4952, Bibcode:2011A&A...531A.165P, doi:10.1051/0004-6361/201116769, S2CID 54940439.
  6. "2 Sex". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2019-04-08.
  7. 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.
  8. Morton Wagman (2003). Lost Stars: Lost, Missing, and Troublesome Stars from the Catalogues of Johannes Bayer, Nicholas-Louis de Lacaille, John Flamsteed, and Sundry Others (2 ed.). McDonald & Woodward Publishing Company. ISBN 978-0-939923-78-6. OCLC 1131243914.
  9. Lépine, Sébastien; Shara, Michael M. (March 2005), "A Catalog of Northern Stars with Annual Proper Motions Larger than 0.15" (LSPM-NORTH Catalog)", The Astronomical Journal, 129 (3): 1483–1522, arXiv:astro-ph/0412070, Bibcode:2005AJ....129.1483L, doi:10.1086/427854, S2CID 2603568.