Phosphine on Jupiter and implications for the Great Red SPOT

Computer Science

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Atmospheric Chemistry, Jupiter Atmosphere, Jupiter Red Spot, Phosphines, Atmospheric Models, Atmospheric Turbulence, Photochemical Reactions, Turbulent Mixing

Scientific paper

A study of the chemistry and photochemistry of the recently discovered phosphine in the atmosphere of Jupiter suggests that the red colorations on this planet result from photochemical production of red phosphorus particles. Chemical-dynamical models of this red phosphorus haze imply that the intensity of the red coloration is a strong function of the strength of vertical turbulent mixing in the atmosphere. If the Jovian Great Red Spot is a region of considerable dynamical activity our model provides a self-consistent explanation for the redness of this region in comparison to the rest of the planet.

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