Higher methane in simulated Pluto atmospheres increases haze production and changes nitrogen bonding from cyanides to amines in the resulting organic solids.
The red, green, and yellow colors correspond to the CHO, CHN, and CHON subgroups, respectively
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Seasonal Variability of Pluto's Haze Formation Revealed by Laboratory Simulations
Higher methane in simulated Pluto atmospheres increases haze production and changes nitrogen bonding from cyanides to amines in the resulting organic solids.