WASP-4b
Template:Short description Script error: No such module "infobox".Script error: No such module "Check for unknown parameters". WASP-4b is an exoplanet, specifically a hot Jupiter, approximately 891 light-years away[1] in the constellation of Phoenix.[2]
Discovery
The planet was the discovered by the Wide Angle Search for Planets team using images taken with the SuperWASP-South project's eight wide-angle cameras located at the South African Astronomical Observatory.[3][4][5] Analysis of over 4000 images taken between May and November 2006 resulted in the detection of a transit occurring every 1.3 days. Follow-up radial velocity observations using the Swiss 1.2-metre Leonhard Euler Telescope confirmed that the transiting object was a planet.[5]
Characteristics
The planetary equilibrium temperature would be 1650±30 K,[6] but the measured dayside temperature is higher, with a 2015 study finding 1900±100 K[7] and a 2020 study finding 1957±68 K.[8]
A study in 2012, utilizing the Rossiter–McLaughlin effect, determined the planetary orbit is probably aligned with the equatorial plane of the star, with misalignment equal to -1Script error: No such module "Su".°.[9]
Orbital decay and tidal interactions
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. The anomalously high rate of orbital decay of WASP-4b was poorly understood as of 2021.[10] In 2025, the planet has been confirmed to have its orbit in decay. This decay is primarily driven by tidal interactions between the planet and its star. Studies based on Transit timing variations (TTVs) indicate that the planet’s orbit is shrinking due to energy dissipation caused by stellar tides. A tidal quality factor of approximately 80,000 was derived from these observations, suggesting that the star is more evolved than previously thought. This phenomenon is consistent with a model of tidal dissipation involving internal gravity waves within the star, although further modeling of the star's properties is needed for a complete understanding.[11]
References
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- ↑ Table 3, Improved parameters for the transiting hot Jupiters WASP-4b and WASP-5b, M. Gillon et al., Astronomy and Astrophysics 496, #1 (2009), pp. 259–267, Script error: No such module "CS1 identifiers"., Bibcode:2009A&A...496..259GScript error: No such module "check bibcode"..
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Further reading
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External links
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