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We developed a 1D photo-thermochemical model to study the atmosphere of warmexoplanets. The chemical scheme used in this model is completely new inplanetology and has been constructed in collaboration with specialists ofcombustion. It has been validated as a whole through experiments on a largerange of temperature (300 - 2500 K) and pressure (1 mbar - 100 bar), allowingto study a wide variety of exoplanets. We have used this chemical model tostudy the atmosphere of two warm Neptunes, GJ3470b and GJ436b, and theinfluence of different parameters (vertical mixing, metallicity, temperature, .. . ) on their chemical composition. We present here the results obtained inthese studies.

Influence of different parameters on the chemical composition of warm neptunes