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HD 192263 is an 8th magnitude star about 64 light years away[8] in the constellation of Aquila. The spectral type of the star is K2V, meaning that it is an orange dwarf, a type of star somewhat cooler and less luminous than the Sun. It is not visible to the unaided eye, but with good binoculars or small telescope it should be easy to spot.

HD 192263

The b+y band light curve for HD 192263, adapted from Dragomir et al. (2012)[1]
Observation data
Epoch J2000      Equinox J2000
Constellation Aquila
Right ascension 20h 13m 59.84551s[2]
Declination −00° 52′ 00.7717″[2]
Apparent magnitude (V) 7.79[3]
Characteristics
Spectral type K1/2 V[4]
B−V color index 0.938±0.015[3]
Variable type BY Draconis variable[5]
Astrometry
Radial velocity (Rv)−10.67±0.09[3] km/s
Proper motion (μ) RA: −62.671[3] mas/yr
Dec.: +260.961[3] mas/yr
Parallax (π)50.8982 ± 0.0561 mas[3]
Distance64.08 ± 0.07 ly
(19.65 ± 0.02 pc)
Absolute magnitude (MV)6.36[3]
Details[6]
Mass0.65±0.09 M☉
Radius0.74±0.02 R☉
Luminosity0.295+0.014
−0.013 L☉
Surface gravity (log g)4.51 cgs
Temperature4,955 K
Metallicity [Fe/H]+0.08 dex
Age6.6+4.7
−4.4 Gyr
Other designations
Phoenicia, V1703 Aquilae, BD−01° 3925, HD 192263, HIP 99711, HR 7288, SAO 144192, LTT 8003, NLTT 48902[7]
Database references
SIMBADdata
ARICNSdata
Extrasolar Planets
Encyclopaedia		data

The star HD 192263 is named Phoenicia. The name was selected in the NameExoWorlds campaign by Lebanon, during the 100th anniversary of the IAU. Phoenicia was an ancient thalassocratic civilisation of the Mediterranean that originated from the area of modern-day Lebanon.[9][10]

Various companions for the star have been reported, but all of them are probably line-of-sight optical components or just spurious observations.

The apparent direction of the star lies close to the Earth's Celestial equator, and it rotates almost edge-on to Earth's line of sight.[11]

In 1999 an extrasolar planet was announced orbiting the star.


Planetary system


On 28 September 1999, a planet around HD 192263 was found by the Geneva Extrasolar Planet Search team using the CORALIE spectrograph on the 1.2m Euler Swiss Telescope at La Silla Observatory,[12] discovered independently by Vogt et al.[13]

The HD 192263 planetary system[1]
Companion
(in order from star)		 Mass Semimajor axis
(AU)		 Orbital period
(days)		 Eccentricity Inclination Radius
b >0.641±0.61 MJ 0.15312±0.00095 24.3587±0.0022 0.008±0.014 — —

See also



References


  1. Dragomir, Diana; et al. (2012). "The HD 192263 System: Planetary Orbital Period and Stellar Variability Disentangled". The Astrophysical Journal. 754 (1). 37. arXiv:1206.2103. Bibcode:2012ApJ...754...37D. doi:10.1088/0004-637X/754/1/37. S2CID 15036240.
  2. Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv:1804.09365. Bibcode:2018A&A...616A...1G. doi:10.1051/0004-6361/201833051.
  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, S2CID 119257644.
  4. Houk, N.; Swift, C. (1999), "Michigan catalogue of two-dimensional spectral types for the HD Stars", Michigan Spectral Survey, Ann Arbor, Michigan: Department of Astronomy, University of Michigan, 5, Bibcode:1999MSS...C05....0H
  5. Samus, N. N.; et al. (2017), "General Catalogue of Variable Stars", Astronomy Reports, GCVS 5.1, 61 (1): 80–88, Bibcode:2017ARep...61...80S, doi:10.1134/S1063772917010085, S2CID 125853869.
  6. Brewer, John M.; et al. (2016), "Spectral Properties of Cool Stars: Extended Abundance Analysis of 1,617 Planet-Search Stars", The Astrophysical Journal Supplement Series, 225 (2): 32, arXiv:1606.07929, Bibcode:2016ApJS..225...32B, doi:10.3847/0067-0049/225/2/32, S2CID 118507965.
  7. "HD 192263". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved November 8, 2018.
  8. Brown, A. G. A; et al. (2016). "Gaia Data Release 1. Summary of the astrometric, photometric, and survey properties". Astronomy and Astrophysics. 595. A2. arXiv:1609.04172. Bibcode:2016A&A...595A...2G. doi:10.1051/0004-6361/201629512. S2CID 1828208.Gaia Data Release 1 catalog entry
  9. "Approved names". NameExoworlds. Retrieved 2020-01-02.
  10. "International Astronomical Union | IAU". www.iau.org. Retrieved 2020-01-02.
  11. Santos, N. C.; et al. (2003). "The CORALIE survey for southern extra-solar planets XI. The return of the giant planet orbiting HD 192263". Astronomy and Astrophysics. 406 (1): 373–381. arXiv:astro-ph/0305434. Bibcode:2003A&A...406..373S. doi:10.1051/0004-6361:20030776. S2CID 16247618.
  12. Santos, N. C.; et al. (2000). "The CORALIE survey for Southern extra-solar planets III. A giant planet in orbit around HD 192263". Astronomy and Astrophysics. 356: 599–602. Bibcode:2000A&A...356..599S. Archived from the original on 2011-09-28. Retrieved 2006-06-04.
  13. Vogt, Steven S.; et al. (2000). "Six New Planets from the Keck Precision Velocity Survey". The Astrophysical Journal. 536 (2): 902–914. arXiv:astro-ph/9911506. Bibcode:2000ApJ...536..902V. doi:10.1086/308981. S2CID 119375519.



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На других языках

[de] HD 192263

HD 192263 ist ein Stern der achten Helligkeitsklasse im Sternbild Aquila. Es handelt sich um einen Hauptreihenstern der Spektralklasse K0. Der Stern ist somit etwas kühler und etwas weniger hell als unsere Sonne. Mit sehr guten Ferngläsern und Teleskopen ist der Stern nachts gut auszumachen. HD 192263 ist ein BY-Draconis-Veränderlicher.
- [en] HD 192263

[es] HD 192263

HD 192263 es una estrella de 8.ª magnitud situada en la constelación de Aquila. El tipo espectral de la estrella es K2V, por lo que se trata de una enana naranja, un tipo de estrella más fría y menos luminosa que el Sol. No es posible observarla a simple vista, pero con unos simples prismáticos o con un pequeño telescopio debería ser fácilmente localizable. La estrella se encuentra muy cerca del ecuador terrestre.


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