Jupiter's Ammonia Hailstorms: A Deep Dive into the Giant Planet's Atmosphere
Scientists at UC Berkeley have confirmed the existence of ammonia-water 'mushballs' on Jupiter – icy slushballs that act like hailstones during thunderstorms. This discovery stems from explaining the uneven distribution of ammonia gas in Jupiter's upper atmosphere, confirmed by data from NASA's Juno mission and Earth-based radio telescopes, and a newly created 3D visualization of Jupiter's upper atmosphere. The mushballs penetrate deep into Jupiter's atmosphere, altering our understanding of the mixing in giant planet atmospheres and offering insights into the internal structure of other gas giants and even exoplanets. The research challenges the long-held assumption of a well-mixed Jovian atmosphere, revealing the crucial role of deep storms and mushballs in redistributing materials.