IAA authors:
Lopez-Valverde, M. A.;Brines, A.;Lopez-Moreno, J. J.
Authors:
Aoki, S.;Shiobara, K.;Yoshida, N.;Trompet, L.;Yoshida, T.;Terada, N.;Nakagawa, H.;Liuzzi, G.;Vandaele, A. C.;Thomas, I. R.;Villanueva, G. L.;Lopez-Valverde, M. A.;Brines, A.;Patel, M. R.;Faggi, S.;Daerden, F.;Erwin, J. T.;Ristic, B.;Bellucci, G.;Lopez-Moreno, J. J.;Kurokawa, H.;Ueno, Y.
Journal:
The Planetary Science Journal
Abstract:
The atmosphere of Mars is mainly composed by carbon dioxide (CO<SUB>2</SUB>). It has been predicted that photodissociation of CO<SUB>2</SUB> depletes <SUP>13</SUP>C in carbon monoxide (CO). We present the carbon <SUP>13</SUP>C/<SUP>12</SUP>C isotopic ratio in CO at 30-50 km altitude from the analysis of the solar occultation measurements taken by the instrument Nadir and Occultation for Mars Discovery on board the ExoMars Trace Gas Orbiter (ExoMars-TGO). We retrieve <SUP>12</SUP>C<SUP>16</SUP>O, <SUP>13</SUP>C<SUP>16</SUP>O, and <SUP>12</SUP>C<SUP>18</SUP>O volume mixing ratios from the spectra taken at 4112-4213 cm<SUP>-1</SUP>, where multiple CO isotope lines with similar intensities are available. The intensities of the <SUP>12</SUP>C<SUP>16</SUP>O lines in this spectral range are particularly sensitive to temperature, thus we derive the atmospheric temperature by retrieving CO<SUB>2</SUB> density with simultaneously measured spectra at 2966-2990 cm<SUP>-1</SUP>. The mean δ <SUP>13</SUP>C value obtained from the <SUP>13</SUP>C<SUP>16</SUP>O/<SUP>12</SUP>C<SUP>16</SUP>O ratios is -263‰, and the standard deviation and standard error of the mean are 132‰ and 4‰, respectively. The relatively large standard deviation is due to the strong temperature dependences in the <SUP>12</SUP>C<SUP>16</SUP>O lines. We also examine the <SUP>13</SUP>C<SUP>16</SUP>O/<SUP>12</SUP>C<SUP>18</SUP>O ratio, whose lines are less sensitive to temperature. The mean δ value obtained with <SUP>12</SUP>C<SUP>18</SUP>O instead of <SUP>12</SUP>C<SUP>16</SUP>O is -82‰ with smaller standard deviation, 60‰. These results suggest that CO is depleted in <SUP>13</SUP>C when compared to CO<SUB>2</SUB> in the Martian atmosphere as measured by the Curiosity rover. This depletion of <SUP>13</SUP>C in CO is consistent with the CO<SUB>2</SUB> photolysis-induced fractionation, which might support a CO-based photochemical origin of organics in Martian sediments.
URL:
https://ui.adsabs.harvard.edu/#abs/2023PSJ.....4...97A/abstract
Keywords:
Planetary atmospheres;1244