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Supersolar Metallicity and Tentative Evidence for Photochemistry on WASP-96 b from JWST and Ground-based VLT Transmission Spectroscopy

  • Authors: Michael Radica, Jake Taylor, Yoav Rotman, Jasmina Blecic, Luis Welbanks, Eva-Maria Ahrer, Duncan Christie, Louis-Philippe Coulombe, Gillis Lowry, Matthew M. Murphy, Adina D. Feinstein, David Lafrenière, Ryan J. MacDonald, Nathan J. Mayne, Shang-Min Tsai, Maria Zamyatina

Michael Radica et al 2026 The Astronomical Journal 171 .

  • Provider: AAS Journals

Caption: Figure 7.

PT profiles derived from cloud-free UM GCM simulations of WASP-96 b at solar (bottom) and 10× solar (top) metallicity, which bracket our derived atmosphere composition. Blue and red profiles represent the morning and evening hemispheres, respectively. Levels of fading denote latitude, with the boldest colors being polar latitudes. Condensation curves for prominent condensate species (labeled) are shown with gray dashed lines.

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