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WASP-96b

Gas giant exoplanet targeted for spectroscopy From Wikipedia, the free encyclopedia

WASP-96b
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WASP-96b is a gas giant exoplanet. Its mass is 0.48 times that of Jupiter. It is 0.0453 AU from the class G star WASP-96, which it orbits every 3.4 days. It is about 1,140 light-years away from Earth, in the constellation Phoenix. It was discovered in 2013 by the Wide Angle Search for Planets (WASP).

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WASP-96b orbits its Sun-like star WASP-96 every 3.4 Earth days at a distance just one-ninth of the distance between Mercury and the Sun.[3]

The hot-Jupiter exoplanet was found via the transiting method by Coel Hellier et.al. in 2013 as part of the WASP-South survey.[1]

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Atmosphere

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WASP-96b's spectrum was one of the images featured in the initial science release from the James Webb Space Telescope in July 2022.[4] The spectrum confirmed the presence of water, as well as providing evidence for "clouds and hazes" within the planet's atmosphere.[3] Prior to this discovery, WASP-96b was thought to be free of clouds.[5][6]

While the light curve released confirms properties of the planet that had already been determined from other observations – the existence, size, and orbit of the planet – the transmission spectrum revealed previously hidden details of the atmosphere: the unambiguous signature of water, indications of haze, and evidence of clouds that were suspected based on prior observations.[7]

A study in 2023 measured the abundance of certain chemical species in the atmosphere of WASP-96b as seen in the table below.[8] Models of the atmosphere with patchy clouds and hazes best describes the observations through the James Webb Space Telescope.[8]

More information Chemical Species, log(VMR) ...
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References

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