Astronomers have analysed the ambiance of WASP-166 b, a sizzling super-Neptune exoplanet, revealing the presence of water and carbon dioxide. Using knowledge from the James Webb Space Telescope (JWST), the observations additionally detected ammonia in smaller portions. WASP-166 b is located roughly 368 light-years away and is about seven instances bigger and 32 instances heavier than Earth. The planet, orbiting its host star each 5.44 days at a distance of 0.067 AU, has an estimated equilibrium temperature of 1,270 Okay, putting it inside the sizzling Neptune desert.
Findings from JWST Observations
As reported by phys.org, the JWST employed its Near Infrared Imager and Slitless Spectrograph (NIRISS) and Near Infrared Camera (NIRCam) to review WASP-166 b’s ambiance. These observations highlighted water and carbon dioxide as dominant components within the spectrum, alongside weak traces of ammonia and cloud deck strain. Helium and hydrogen, in a primordial photo voltaic ratio, are believed to compose the remaining ambiance. Searches for compounds like carbon monoxide yielded no vital outcomes.
Characteristics of WASP-166 and Its Planet
WASP-166, the host star of this exoplanet, belongs to the F9V spectral sort and is roughly 20 p.c bigger and extra huge than the solar. It is 2.1 billion years outdated, with a floor temperature of 6,050 Okay and a metallicity of 0.19 dex. The planetary carbon-to-oxygen ratio of WASP-166 b was calculated to be 0.282, considerably decrease than each the host star (0.41) and the solar (0.55). Additionally, the planet’s excessive atmospheric metallicity of 1.57 was reported.
Explanations for Atmospheric Composition
It was instructed that the atmospheric composition might be linked to planetesimal accretion, core erosion, or photoevaporation. Such findings contribute to understanding planetary formation and evolution, notably inside areas like the recent Neptune desert. The examine offers insights into the range of exoplanetary programs and their distinctive traits.
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