File:WASP18b Spectrum print.tif

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English: The team of researchers obtained the thermal emission spectrum of WASP-18 b by measuring the amount of light it emits over NASA’s James Webb Space Telescope’s NIRISS SOSS 0.85-2.8 um wavelength range, capturing 65% of the total energy emitted by the planet. WASP-18 b is so hot on the day side of this tidally-locked planet (the same side always faces its star, as the Moon to Earth) that water vapor molecules would break apart. The Webb Telescope directly observed water vapor on the planet in even relatively small amounts, indicating the sensitivity of the observatory.
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Source https://exoplanets.nasa.gov/resources/2349/wasp-18-b-atmospheric-spectrum-from-james-webb-space-telescope/
Author NASA/JPL-Caltech (R. Hurt/IPAC)

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Public domain This file is in the public domain in the United States because it was solely created by NASA. NASA copyright policy states that "NASA material is not protected by copyright unless noted". (See Template:PD-USGov, NASA copyright policy page or JPL Image Use Policy.)
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current07:11, 11 July 2023Thumbnail for version as of 07:11, 11 July 20233,840 × 2,160 (1.81 MB)Юрий Д.К. (talk | contribs)Uploaded a work by NASA/JPL-Caltech (R. Hurt/IPAC) from https://exoplanets.nasa.gov/resources/2349/wasp-18-b-atmospheric-spectrum-from-james-webb-space-telescope/ with UploadWizard

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