Saturn's Atmosphere in Northern Summer Revealed by JWST/MIRI
Leigh N. Fletcher, Oliver R.T. King, Jake Harkett, Heidi B. Hammel,, Michael T. Roman, Henrik Melin, Matthew M. Hedman, Julianne I. Moses,, Sandrine Guerlet, Stefanie N. Milam, Matthew S. Tiscareno

TL;DR
This study uses JWST/MIRI to map Saturn's northern summer atmosphere, revealing temperature, chemical, and aerosol variations, including new insights into stratospheric composition, dynamics, and seasonal evolution since the Cassini mission.
Contribution
First spectral mapping of Saturn's northern hemisphere in the 5-28 μm range, providing new data on atmospheric composition, aerosols, and wind patterns post-Cassini.
Findings
Ammonia shows equatorial enrichment, indicating similar dynamics to Jupiter.
Saturn's North Polar Vortex has warmed and shows hydrocarbon enhancements.
Latitudinal temperature gradients align with zonal wind peaks.
Abstract
Saturn's northern summertime hemisphere was mapped by JWST/MIRI (4.9-27.9 m) in November 2022, tracing the seasonal evolution of temperatures, aerosols, and chemical species in the five years since the end of the Cassini mission. The spectral region between reflected sunlight and thermal emission (5.1-6.8 m) is mapped for the first time, enabling retrievals of phosphine, ammonia, and water, alongside a system of two aerosol layers (an upper tropospheric haze bars, and a deeper cloud layer at 1-2 bars). Ammonia displays substantial equatorial enrichment, suggesting similar dynamical processes to those found in Jupiter's equatorial zone. Saturn's North Polar Stratospheric Vortex has warmed since 2017, entrained by westward winds at mbar, and exhibits localised enhancements in several hydrocarbons. The strongest latitudinal temperature gradients are co-located with…
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