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WASP-5

Coordinates:Sky map23h 57m 23.759s, −41° 16′ 37.74″
From Wikipedia, the free encyclopedia
WASP-5
Observation data
EpochJ2000.0      EquinoxJ2000.0
ConstellationPhoenix
Right ascension23h 57m 23.75647s[1]
Declination−41° 16′ 37.7437″[1]
Apparent magnitude (V)12.146[2]
Characteristics
Evolutionary stageMain sequence
Spectral typeG4V[3]
Apparent magnitude (B)12.808±0.02[2]
Apparent magnitude (V)12.146±0.01[2]
Apparent magnitude (J)10.949±0.022[2]
Apparent magnitude (H)10.650±0.025[2]
Apparent magnitude (K)10.598±0.023[2]
Astrometry
Radial velocity (Rv)20.49±0.67[1] km/s
Proper motion (μ)RA: 7.406(14)mas/yr[1]
Dec.: −16.072(14)mas/yr[1]
Parallax (π)3.1883±0.0150 mas[1]
Distance1,023 ± 5 ly
(314 ± 1 pc)
Details[4]
Mass1.033±0.045 M
Radius1.088±0.040 R
Temperature5770±65 K
Metallicity [Fe/H]0.090±0.090 dex
Rotation16.20±0.40 d
Rotational velocity (v sin i)3.40±0.70 km/s
Age5.84±1.86[5] Gyr
Other designations
TOI-250,TIC 184240683,WASP-5,GSC 08018-00199,2MASS J23572375-4116377,DENIS J235723.7-411637, UCAC2 14323784[2]
Database references
SIMBADdata

WASP-5 is amagnitude 12G-type main-sequence star located about 1,020light-years (310parsecs) away in thePhoenixconstellation.[2] The star is likely older than the Sun, slightly enriched in heavy elements and is rotating rapidly, being spun up by the tides raised by the giant planet on a close orbit.[5]

Planetary system

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This star has oneexoplanet,WASP-5b, detected by theSuperWASP project in 2007.[3]

The WASP-5 planetary system[4]
Companion
(in order from star)
MassSemimajor axis
(AU)
Orbital period
(days)
EccentricityInclinationRadius
b1.590+0.053
−0.052
 MJ
0.02739±0.000391.62842953(52)<0.01285.8±1.1°1.175±0.056 RJ

See also

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References

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  1. ^abcdeVallenari, A.; et al. (Gaia collaboration) (2023)."Gaia Data Release 3. Summary of the content and survey properties".Astronomy and Astrophysics.674: A1.arXiv:2208.00211.Bibcode:2023A&A...674A...1G.doi:10.1051/0004-6361/202243940.S2CID 244398875. Gaia DR3 record for this source atVizieR.
  2. ^abcdefgh"WASP-5".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved14 December 2023.
  3. ^abAnderson, D.R.; Gillon, M.; Hellier, C.; Maxted, P. F. L.; Pepe, F.; Queloz, D.; Wilson, D. M.; Collier Cameron, A.; Smalley, B.; Lister, T. A.; Bentley, S. J.; Blecha, A.; Christian, D. J.; Enoch, B.; Hebb, L.; Horne, K.; Irwin, J.; Joshi, Y. C.; Kane, S. R.; Marmier, M.; Mayor, M.; Parley, N. R.; Pollacco, D. L.; Pont, F.; Ryans, R.; Ségransan, D.; Skillen, I.; Street, R. A.; Udry, S.; et al. (2008)."WASP-5b: a dense, very hot Jupiter transiting a 12th-mag Southern-hemisphere star".Monthly Notices of the Royal Astronomical Society: Letters.387 (1):L4 –L7.arXiv:0801.1685.Bibcode:2008MNRAS.387L...4A.doi:10.1111/j.1745-3933.2008.00465.x.S2CID 36741190.
  4. ^abBonomo, A. S.; Desidera, S.; et al. (June 2017). "The GAPS Programme with HARPS-N at TNG. XIV. Investigating giant planet migration history via improved eccentricity and mass determination for 231 transiting planets".Astronomy & Astrophysics.602: A107.arXiv:1704.00373.Bibcode:2017A&A...602A.107B.doi:10.1051/0004-6361/201629882.S2CID 118923163.
  5. ^abMaxted, P. F. L.; Serenelli, A. M.; Southworth, J. (2015), "A comparison of gyrochronological and isochronal age estimates for transiting exoplanet host stars",Astronomy & Astrophysics,577: A90,arXiv:1503.09111,Bibcode:2015A&A...577A..90M,doi:10.1051/0004-6361/201525774,S2CID 53324330

External links

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