WASP-14orBD+22 2716is a star in the constellationBoötes.TheSuperWASPproject has observed and classified this star as avariable star,perhaps due to theeclipsingplanet.[2]

WASP-14
Observation data
EpochJ2000EquinoxJ2000
Constellation Boötes
Right ascension 14h33m06.3574s[1]
Declination +21° 53′ 40.975″[1]
Apparent magnitude(V) 9.745 ± 0.026
Characteristics
Spectral type F5V
Variable type V*(1SWASP)[2]
Astrometry
Proper motion(μ)RA:28.7±0.6[3]mas/yr
Dec.:−6.6±0.8[3]mas/yr
Parallax(π)6.1442 ± 0.0305mas[2]
Distance531 ± 3ly
(162.8 ± 0.8pc)
Absolute magnitude(MV)10.194 ± 0.029
Details
Mass~1.319M
Radius~1.297R
Luminosity2.61L
Surface gravity(logg)~21,9gcgs
Temperature6475 ± 100K
Metallicity[Fe/H]0 ± 0.2dex
Age750 ± 250Myr
Other designations
BD+22° 2716,2MASSJ14330635+2153409,PPM103396,TYC1482-882-1,GSC01482-00882,SAO83398, Gaia DR2 1242084170974175232
Database references
SIMBADdata
Data sources:
Hipparcos Catalogue,
CCDM(2002),
Bright Star Catalogue (5th rev. ed.)

Planetary system

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WASP-14bis anextrasolar planetdiscovered in 2008. This is one of the densest exoplanets known.[4] Its radius best fits the model of Fortney.[5]

The WASP-14 planetary system
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
b ~7.725MJ ~0.037 ~2.243756 ~0.095 84.79° 1.259RJ

See also

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References

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  1. ^abBrown, 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.S2CID1828208.Gaia Data Release 1 catalog entry
  2. ^abc"SIMBAD query result: BD+22 2716 -- Star".Centre de Données astronomiques de Strasbourg.Retrieved2009-05-04.
  3. ^abZacharias, N.; et al. (2013). "The Fourth US Naval Observatory CCD Astrograph Catalog (UCAC4)".The Astronomical Journal.145(2). 44.arXiv:1212.6182.Bibcode:2013AJ....145...44Z.doi:10.1088/0004-6256/145/2/44.S2CID119299381.Vizier catalog entry
  4. ^Joshi, Y. C.; et al. (2008)."WASP-14b: A 7.7 Mjup transiting exoplanet in an eccentric orbit".Monthly Notices of the Royal Astronomical Society.392(4): 1532–1538.arXiv:0806.1478.Bibcode:2009MNRAS.392.1532J.doi:10.1111/j.1365-2966.2008.14178.x.S2CID7775011.
  5. ^Fortney; Marley, M. S.; Barnes, J. W. (2007). "Planetary Radii across Five Orders of Magnitude in Mass and Stellar Insolation: Application to Transits".The Astrophysical Journal.659(2): 1661–1672.arXiv:astro-ph/0612671.Bibcode:2007ApJ...659.1661F.doi:10.1086/512120.S2CID3039909.
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