Javascript must be enabled to continue!
Saturn
View through CrossRef
This chapter compares the climate of Saturn with that of Jupiter. Both Jupiter and Saturn have no oceans and no solid surfaces, but they have lightning storms and rain clouds that dwarf the largest thunderstorms on Earth. Saturn's weather is normally very calm, but every 20–30 years a giant storm erupts. These storms last for a few months and then disappear. In contrast, Jupiter's giant storms endure without change for decades or centuries. Saturn's winds are stronger than Jupiter's. The chapter first reviews the variables that might control the planets' climates before discussing how the climates actually differ. It examines Saturn's rotation, giant storms, effective radiating temperature, electrostatic discharges and lightning, enrichment relative to solar composition, helium raindrops, moist convection and conditional instability, and ortho-para instability.
Title: Saturn
Description:
This chapter compares the climate of Saturn with that of Jupiter.
Both Jupiter and Saturn have no oceans and no solid surfaces, but they have lightning storms and rain clouds that dwarf the largest thunderstorms on Earth.
Saturn's weather is normally very calm, but every 20–30 years a giant storm erupts.
These storms last for a few months and then disappear.
In contrast, Jupiter's giant storms endure without change for decades or centuries.
Saturn's winds are stronger than Jupiter's.
The chapter first reviews the variables that might control the planets' climates before discussing how the climates actually differ.
It examines Saturn's rotation, giant storms, effective radiating temperature, electrostatic discharges and lightning, enrichment relative to solar composition, helium raindrops, moist convection and conditional instability, and ortho-para instability.
Related Results
Towards long-term simulations of planetary-scale vortices and storms on Jupiter and Saturn
Towards long-term simulations of planetary-scale vortices and storms on Jupiter and Saturn
Long-term simulations of planetary vortices and storms are essential for improving our understanding of the atmospheric dynamics on gas giants such as Jupiter and Saturn. These sim...
Saturn’s atmospheric winds between 2021 and 2024
Saturn’s atmospheric winds between 2021 and 2024
Saturn’s zonal wind profile at cloud level has been measured at different epochs since the first spacecraft visits from Voyager 1 and 2 in 1980-81 [1-2]. Saturn’s wind measurements...
Survey of Irregular Jovian Moons with IVO
Survey of Irregular Jovian Moons with IVO
The Io Volcano Observer (IVO) [1] is a NASA Discovery mission currently under Phase A study [2]. Its primary goal is a thorough investigation of Io (e.g., [3]), the innermost of Ju...
Micrometeoroid Pollution Resistance Sustains the Pristine—and Possibly Ancient—Rings of Saturn
Micrometeoroid Pollution Resistance Sustains the Pristine—and Possibly Ancient—Rings of Saturn
Saturn’s rings have been considered youthful—no more than a few × 108 years—because dark, non-icy micrometeoroids should steadily accumulate on the predominantly water-ice ring par...
Direct stratospheric wind measurements with ALMA during Saturn's 2010-2013 Great Storm
Direct stratospheric wind measurements with ALMA during Saturn's 2010-2013 Great Storm
Great White Spot events occur every orbital period in Saturn's atmosphere (Sanchez-Lavega et al. 2018). These planetary scale storms perturb the upper tropospheric cloud deck for w...
The Midsized Moons of Saturn
The Midsized Moons of Saturn
The midsized, icy moons of Saturn—Mimas, Enceladus, Tethys, Dione, Rhea, and Iapetus—are each remarkable worlds and together form a fascinating system. The innermost of these bodie...
Recent advances on magnetic reconnection and dipolarization at Saturn
Recent advances on magnetic reconnection and dipolarization at Saturn
<p>Magnetic reconnection and dipolarization are crucial processes in driving magnetospheric dynamics, including particle energization, mass circulation, auroral proce...
Is Saturn a failed gas giant?
Is Saturn a failed gas giant?
The formation history of giant planets inside and outside the Solar System remains unknown. We suggest that runaway gas accretion is initiated only at a mass of ∼100 M&am...

