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# Program information file
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PROGRAM_ID           2023A081
PROGRAM_TITLE        CO and its isotopologues at Venus cloud top: Tracer for atmospheric chemistry and dynamics
PROGRAM_INV1         Hideo Sagawa
PROGRAM_INV2         Takao Sato
PROGRAM_INV3         Shohei Aoki
PROGRAM_INV4          
PROGRAM_INV5          
PROGRAM_SCICAT       major planets / satellites
PROGRAM_ABSTRACT_BEG
Carbon dioxide [CO2] in the Venusian atmosphere is photodissociated into carbon monoxide [CO] and oxygen by solar UV radiation. However, the reaction pathway that restores the dissociated CO to CO2 is still unknown. This well-known issue of 'Chemical stability of CO2 atmosphere' is a long-standing unsolved problem, not only for Venus and Mars atmospheres but also for exoplanetary terrestrial planets. 
This proposal will tackle this fundamental problem by observing 13CO/12CO isotopic fractionation for the first time at the Venus cloud-top altitude. The isotopic fractionation of CO can be used to evaluate how effective the CO2 photolysis occurs in Venus, and also to potentially constrain the atmospheric circulation in the Venusian upper atmosphere.
PROGRAM_ABSTRACT_END