Giant Planet Atmospheres

Abstract

The giant planets, Jupiter, Saturn, Uranus, and Neptune, all have vibrant and dynamic atmospheres. The iconic belt--zone structure of Jupiter, together with the Great Red Spot, is instantly recognizable. Saturn, with its dramatic ring system and more muted atmosphere, is a formidable jewel in the Solar System. In the outer reaches, the pale blue Uranus and Neptune are found, worlds about which ultimately very little is known. The atmospheres of these planets are dominated by hydrogen and helium, and unlike the Earth, they do not have a solid surface. These differences generate inherently different types of atmospheres, but there are also similarities. For example, the condensation of water, which forms the familiar clouds on Earth, also occurs on the giant planets. Broadly speaking, the atmosphere can be divided into different regimes defined by their temperature gradients. In the troposphere, where weather occurs, the temperatures decrease as a function of increasing altitude as convection moves internal heat upward; the rising material expands and cools. Above this region lies the stratosphere, defined by a positive temperature gradient, where hydrocarbons are heated by ultraviolet radiation from the Sun (analogous to ozone heating in the terrestrial stratosphere), which also drives substantial photochemistry. This is followed by a mesosphere that cools as a function of altitude, a region that is ill-defined at the giant planets. Finally, the upper atmosphere connects to the space environment and is heated by both solar extreme ultraviolet light and auroral processes. The giant planets are energized both by internal heat and by solar heating. These energy inputs, along with the fast rotation rates of these planets, drive dynamics by establishing global circulation patterns and generating both waves and instabilities. [...]

References in corpus (14)

• Comparing Jupiter interior structure models to Juno gravity measurements and the role of a dilute core
• Neptune at Summer Solstice: Zonal Mean Temperatures from Ground-Based Observations 2003-2007
• Seasonal stratospheric photochemistry on Uranus and Neptune
• Mid-Infrared Spectroscopy of Uranus from the Spitzer Infrared Spectrometer: 2. Determination of the Mean Composition of the Upper Troposphere and Stratosphere
• A Hexagon in Saturn's Northern Stratosphere Surrounding the Emerging Summertime Polar Vortex
• Uranian Satellite Formation by Evolution of a Water Vapor Disk Generated by a Giant Impact
• Assessing the long-term variability of acetylene and ethane in the stratosphere of Jupiter
• Uranus in Northern Mid-Spring: Persistent Atmospheric Temperatures and Circulations Inferred from Thermal Imaging
• Infrared Characterisation of Jupiter's Equatorial Disturbance Cycle
• Ammonia Abundance Derived from Juno MWR and VLA Observations of Jupiter
• Saturn's Atmosphere in Northern Summer Revealed by JWST/MIRI
• Evolution of Neptune at Near-Infrared Wavelengths from 1994 through 2022
• Doppler wind measurements in Neptune's stratosphere with ALMA
• The Thermal Structure and Composition of Jupiter's Great Red Spot From JWST/MIRI