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Oxygen Isotope Fractionation in the Martian Atmosphere Induced by CO2 Photolysis and O3 Formation

  • Authors: Tatsuya Yoshida, Shohei Aoki, Hiromu Nakagawa, Naoki Terada, Juan Alday, Akinori Hasebe, Yuki Nakamura, Shungo Koyama, Shotaro Sakai, Ryoya Sakata, Ann Carine Vandaele

Tatsuya Yoshida et al 2026 The Planetary Science Journal 7 .

  • Provider: AAS Journals

Caption: Figure 7.

Comparison of measured isotopic profiles of CO from TGO solar occultation observations with model results. The left, middle, and right panels show vertical profiles of 18O/16O in CO, 13C/12C in CO, and 13C16O/12C18O, respectively. The isotopic ratios are normalized to the standard reference values of VSMOW (18O/16O = 2.0052 × 10−3) and Vienna Pee Dee Belemnite (VPDB; 13C/12C = 1.123 × 10−2). The blue lines represent the calculation results: the solid, dashed, and dotted lines correspond to the results with the standard eddy diffusion coefficient, a coefficient one order of magnitude smaller, and a coefficient one order of magnitude larger, respectively. The red and orange bars represent the values retrieved from TGO solar occultation measurements by J. Alday et al. (2023) and S. Aoki et al. (2023), respectively.

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