Astronomy:Kappa1 Sagittarii

From HandWiki
Short description: Star in the constellation Sagittarius


For other stars with this Bayer designation, see κ Sagittarii.
κ1 Sagittarii
Microscopium constellation map.svg
Red circle.svg
Location of κ1 Sagittarii (circled)
Observation data
Equinox J2000.0]] (ICRS)
Constellation Sagittarius
Right ascension  20h 22m 27.50366s[1]
Declination −42° 02′ 58.3648″[1]
Apparent magnitude (V) +5.58[2]
Characteristics
Spectral type A0 V[3]
U−B color index −0.008[2]
B−V color index +0.004[2]
Astrometry
Radial velocity (Rv)−11.6[4] km/s
Proper motion (μ) RA: +41.312[5] mas/yr
Dec.: −83.742[5] mas/yr
Parallax (π)14.6086 ± 0.1738[5] mas
Distance223 ± 3 ly
(68.5 ± 0.8 pc)
Absolute magnitude (MV)1.47[6]
Details
Mass2.23±0.02[7] M☉
Radius1.7[8] R☉
Luminosity27.5[7] L☉
Surface gravity (log g)4.33[9] cgs
Temperature9,962±339[9] K
Rotational velocity (v sin i)79[3] km/s
Age161[9] Myr
Other designations
κ1 Sgr, CD−42°14836, HD 193571, HIP 100469, HR 7779, SAO 230177, WDS J20225-4203[10]
Database references
SIMBADdata

Kappa1 Sagittarii (κ1 Sagittarii) is a solitary,[11] white-hued star in the zodiac constellation of Sagittarius. It has an apparent visual magnitude of +5.58,[2] which is bright enough to be faintly visible to the naked eye. According to the Bortle scale, it can be viewed from dark suburban skies. Based upon an annual parallax shift of 15.12 mas as seen from Earth,[1] this star is located around 223 light years from the Sun. It is advancing in the general direction of the Sun with a radial velocity of −11.6 km/s.[4]

This is an A-type main sequence star with a stellar classification of A0 V.[3] It displays an infrared excess, with the measured radiation indicating the star is orbited by a two-component debris disk.[8] The star is about 161[9] million years old with 2.23[7] times the mass of the Sun and 1.7[8] times the Sun's radius. It is radiating 27.5 times the Sun's luminosity from its photosphere at an effective temperature of roughly 9,962 K.[9]

There are two visual companions: component B is a magnitude 12.6 star at an angular separation of 39.3 arc seconds along a position angle of 312°, as of 2000; component C is magnitude 11.6 with a separation of 56.8 arc seconds along a position angle of 283°, as of 1999.[12] Neither star is physically associated with Kappa1 Sagittarii.[11]

References

  1. ↑ 1.0 1.1 1.2 van Leeuwen, F. (2007), "Validation of the new Hipparcos reduction", Astronomy and Astrophysics 474 (2): 653–664, doi:10.1051/0004-6361:20078357, Bibcode: 2007A&A...474..653V. 
  2. ↑ 2.0 2.1 2.2 2.3 Cousins, A. W. J. (1983), "UBV photometry of E region standard stars of intermediate brightness", South African Astronomical Observatory Circular 7 (7): 36–46, Bibcode: 1983SAAOC...7...36C. 
  3. ↑ 3.0 3.1 3.2 Royer, F. et al. (February 2007), "Rotational velocities of A-type stars. III. Velocity distributions", Astronomy and Astrophysics 463 (2): 671–682, doi:10.1051/0004-6361:20065224, Bibcode: 2007A&A...463..671R. 
  4. ↑ 4.0 4.1 Evans, D. S. (June 20–24, 1966), "The Revision of the General Catalogue of Radial Velocities", in Batten, Alan Henry; Heard, John Frederick, Determination of Radial Velocities and their Applications, Proceedings of IAU Symposium no. 30, 30, University of Toronto: International Astronomical Union, p. 57, Bibcode: 1967IAUS...30...57E 
  5. ↑ 5.0 5.1 5.2 Brown, A. G. A. (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics 616: A1. doi:10.1051/0004-6361/201833051. Bibcode: 2018A&A...616A...1G.  Gaia DR2 record for this source at VizieR.
  6. ↑ Ammler-von Eiff, Matthias; Reiners, Ansgar (June 2012), "New measurements of rotation and differential rotation in A-F stars: are there two populations of differentially rotating stars?", Astronomy & Astrophysics 542: A116, doi:10.1051/0004-6361/201118724, Bibcode: 2012A&A...542A.116A. 
  7. ↑ 7.0 7.1 7.2 Zorec, J.; Royer, F. (January 2012), "Rotational velocities of A-type stars. IV. Evolution of rotational velocities", Astronomy & Astrophysics 537: A120, doi:10.1051/0004-6361/201117691, Bibcode: 2012A&A...537A.120Z. 
  8. ↑ 8.0 8.1 8.2 Patel, Rahul I. et al. (February 2017), "The Faintest WISE Debris Disks: Enhanced Methods for Detection and Verification", The Astronomical Journal 153 (2): 19, doi:10.3847/1538-3881/153/2/54, 54, Bibcode: 2017AJ....153...54P. 
  9. ↑ 9.0 9.1 9.2 9.3 9.4 David, Trevor J.; Hillenbrand, Lynne A. (2015), "The Ages of Early-Type Stars: Strömgren Photometric Methods Calibrated, Validated, Tested, and Applied to Hosts and Prospective Hosts of Directly Imaged Exoplanets", The Astrophysical Journal 804 (2): 146, doi:10.1088/0004-637X/804/2/146, Bibcode: 2015ApJ...804..146D. 
  10. ↑ "kappa01 Sgr". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=kappa01+Sgr. 
  11. ↑ 11.0 11.1 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, doi:10.1111/j.1365-2966.2008.13596.x, Bibcode: 2008MNRAS.389..869E. 
  12. ↑ Mason, B. D. et al. (2014), "The Washington Visual Double Star Catalog", The Astronomical Journal 122 (6): 3466–3471, doi:10.1086/323920, Bibcode: 2001AJ....122.3466M, http://vizier.u-strasbg.fr/viz-bin/VizieR?-source=B/wds, retrieved 2015-07-22. 



Retrieved from "https://handwiki.org/wiki/index.php?title=Astronomy:Kappa1_Sagittarii&oldid=3424075"