Astronomy:WASP-4

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Short description: G-type main sequence star in the constellation Phoenix
WASP-4
Planet WASP-4.png

Artistic rendering of WASP-4 b
Observation data
Equinox J2000.0]] (ICRS)
Constellation Phoenix[1]
Right ascension  23h 34m 15.0857s[2]
Declination −42° 03′ 41.048″[2]
Apparent magnitude (V) 12.468±0.025[3]
Characteristics
Evolutionary stage Main sequence
Spectral type G7V[4]
Apparent magnitude (V) 12.468±0.025[3]
Apparent magnitude (B) 13.216±0.020[3]
Variable type Planetary transit variable[4]
Astrometry
Radial velocity (Rv)57.61±0.76[2] km/s
Proper motion (μ) RA: 9.950(12)[2] mas/yr
Dec.: −87.620(10)[2] mas/yr
Parallax (π)3.6623 ± 0.0147[2] mas
Distance891 ± 4 ly
(273 ± 1 pc)
Details[5]
Mass0.89±0.01 M
Radius0.920±0.060 R
Surface gravity (log g)4.484+0.037−0.047[6] cgs
Temperature5436±34 K
Metallicity [Fe/H]−0.050±0.040 dex
Rotation22.2±3.3 d
Rotational velocity (v sin i)2.2+0.6
−1.0
 km/s
Age7.0±2.9 Gyr
Other designations
1SWASP J233415.06-420341.1, TYC 8017-108-1, 2MASS J23341508-4203411[7]
Database references
SIMBADdata

WASP-4 is a G-type main-sequence star approximately 891 light-years away in the constellation of Phoenix.[4][1][2] Despite its advanced age, the star is rotating rapidly, being spun up by the tides raised by a giant planet on a close orbit.[8]

Planetary system

In 2007 the exoplanet WASP-4b was discovered orbiting this star. With an orbital period of just 1.3 days it is classified as a hot Jupiter.[4] The planet's orbital period appears to be decreasing at a rate of 7.33±0.71 milliseconds per year, suggesting that its orbit is decaying, with a decay timescale of 15.77±1.57 million years. Another superjovian planet in the system is suspected.[9]

The WASP-4 planetary system[9]
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
b 1.164±0.082 MJ 0.02239±0.00084 1.338231587(22) <0.0033[5] 88.02±0.69° 1.312±0.045 RJ
c (unconfirmed) ≥5.47±0.44 MJ 6.82±0.25 7001.0±6.6

See also

  • SuperWASP
  • List of extrasolar planets

References

  1. 1.0 1.1 Roman, Nancy G. (1987). "Identification of a Constellation From a Position". Publications of the Astronomical Society of the Pacific 99 (617): 695–699. doi:10.1086/132034. Bibcode1987PASP...99..695R.  Vizier query form
  2. 2.0 2.1 2.2 2.3 2.4 2.5 Vallenari, A. et al. (2022). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy & Astrophysics. doi:10.1051/0004-6361/202243940  Gaia DR3 record for this source at VizieR.
  3. 3.0 3.1 3.2 Henden, A. A. et al. (2016). "VizieR Online Data Catalog: AAVSO Photometric All Sky Survey (APASS) DR9 (Henden+, 2016)". VizieR On-line Data Catalog: II/336. Originally Published in: 2015AAS...22533616H 2336. Bibcode2016yCat.2336....0H.  Vizier catalog entry
  4. 4.0 4.1 4.2 4.3 Wilson, D. M. et al. (2008). "WASP-4b: A 12th Magnitude Transiting Hot Jupiter in the Southern Hemisphere". The Astrophysical Journal Letters 675 (2): L113–L116. doi:10.1086/586735. Bibcode2008ApJ...675L.113W. 
  5. 5.0 5.1 Bonomo, A. 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. doi:10.1051/0004-6361/201629882. Bibcode2017A&A...602A.107B. 
  6. Dragomir, Diana; Kane, Stephen R.; Pilyavsky, Genady; Mahadevan, Suvrath; Ciardi, David R.; Zachary Gazak, J.; Gelino, Dawn M.; Payne, Alan et al. (2011). "Terms Photometry of Known Transiting Exoplanets". The Astronomical Journal 142 (4): 115. doi:10.1088/0004-6256/142/4/115. Bibcode2011AJ....142..115D. 
  7. "WASP-4". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=WASP-4. 
  8. 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, doi:10.1051/0004-6361/201525774, Bibcode2015A&A...577A..90M 
  9. 9.0 9.1 Turner, Jake D.; Flagg, Laura; Ridden-Harper, Andrew; Jayawardhana, Ray (2022), "Characterizing the WASP-4 System with TESS and Radial Velocity Data: Constraints on the Cause of the Hot Jupiter's Changing Orbit and Evidence of an Outer Planet", The Astronomical Journal 163 (6): 281, doi:10.3847/1538-3881/ac686f, Bibcode2022AJ....163..281T 

External links

Coordinates: Sky map 23h 34m 15.06s, −42° 03′ 41.1″