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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 1.

Rate coefficients of the formation reactions of 18O-bearing ozone (top panel) and 17O-bearing ozone (bottom panel) relative to that of O3 (﹩={k}_{{\rm{O}}+{{\rm{O}}}_{2}+{\rm{M}}}﹩) as a function of temperature. The solid red lines represent the rate coefficients of the reactions between O and O18O (or O17O), and the solid orange lines represent those of the reactions between 18O (or 17O) and O2. The dashed lines represent the branching ratios of the production of symmetric and asymmetric ozone through the reactions between O and O18O (or O17O). The dotted black line represents the value corresponding to no isotopic fractionation.

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