Is the atmosphere of the ultra-hot Jupiter WASP-121b variable?
Quentin Changeat, Jack W. Skinner, James Y-K. Cho, Joonas N\"attil\"a,, Ingo P. Waldmann, Ahmed F. Al-Refaie, Achr\`ene Dyrek, Billy Edwards, Thomas, Mikal-Evans, Max Joshua, Giuseppe Morello, Nour Skaf, Angelos Tsiaras, Olivia, Venot, Kai Hou Yip

TL;DR
This study analyzes Hubble observations of ultra-hot Jupiter WASP-121b, revealing a stable thermal inversion and variable atmospheric features indicative of quasi-periodic weather patterns caused by storms and fronts.
Contribution
It provides the first evidence of atmospheric variability in WASP-121b through detailed analysis and simulations, linking observed signals to dynamic weather phenomena.
Findings
Detection of a stable thermal inversion at ~0.1 bar
Identification of time-varying spectral signatures
Evidence of quasi-periodic weather patterns causing atmospheric changes
Abstract
We present a comprehensive analysis of the Hubble Space Telescope observations of the atmosphere of WASP-121 b, a ultra-hot Jupiter. After reducing the transit, eclipse, and phase-curve observations with a uniform methodology and addressing the biases from instrument systematics, sophisticated atmospheric retrievals are used to extract robust constraints on the thermal structure, chemistry, and cloud properties of the atmosphere. Our analysis shows that the observations are consistent with a strong thermal inversion beginning at ~0.1 bar on the dayside, solar to subsolar metallicity Z (i.e., -0.77 < log(Z) < 0.05), and super-solar C/O ratio (i.e., 0.59 < C/O < 0.87). More importantly, utilizing the high signal-to-noise ratio and repeated observations of the planet, we identify the following unambiguous time-varying signals in the data: i) a shift of the putative hotspot offset between…
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Taxonomy
TopicsAstro and Planetary Science · Stellar, planetary, and galactic studies · Astronomy and Astrophysical Research
