WASP-5

Last updated
WASP-5
Observation data
Epoch J2000.0        Equinox J2000.0
Constellation Phoenix
Right ascension 23h 57m 23.75647s [1]
Declination −41° 16′ 37.7437″ [1]
Apparent magnitude  (V)12.146 [2]
Characteristics
Evolutionary stage Main sequence
Spectral type G4V [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]
Distance 1,023 ± 5  ly
(314 ± 1  pc)
Details [4]
Mass 1.033±0.045  M☉
Radius 1.088±0.040  R☉
Temperature 5770±65  K
Metallicity [Fe/H]0.090±0.090  dex
Rotation 16.20±0.40  d
Rotational velocity (v sin i)3.40±0.70 km/s
Age 5.84±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
SIMBAD data
Exoplanet Archive data

WASP-5 is a magnitude 12 G-type main-sequence star located about 1,020 light-years (310 parsecs ) away in the Phoenix constellation. [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]

Contents

Planetary system

This star has one exoplanet, WASP-5b, detected by the SuperWASP project in 2007. [3]

The WASP-5 planetary system [4]
Companion
(in order from star)		 Mass Semimajor axis
(AU)		 Orbital period
(days)		 Eccentricity Inclination Radius
b 1.590+0.053
−0.052  MJ 		0.02739±0.000391.62842953(52)<0.01285.8±1.1 ° 1.175±0.056  RJ

See also

References

  1. 1 2 3 4 5 6 Vallenari, 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 at VizieR.
  2. 1 2 3 4 5 6 7 8 "WASP-5". SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 14 December 2023.
  3. 1 2 Anderson, 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. 1 2 Bonomo, 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. 1 2 Maxted, 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
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