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1 Ιαν 2020 · All of the giant planet atmospheres contain a temperature minimum located at the tropopause; above that, temperatures increase with height due to the absorption of sunlight by stratospheric aerosols and the methane gas absorption bands (Fig.
23 Ιουν 2023 · The extreme temperature variation and the planet's rapid rotation causes massive storms patterns, including the Great Red Spot, a 190-year-old storm larger than terrestrial planet Earth. Saturn " " Jovian planets all have rings, but none are as spectacular as Saturn's.
The Jovian Planets: These images show the four Jovian planets. In the image of Jupiter, the planet’s strong winds blowing east to west create the banded structure . in the atmosphere. The Saturn image shows the shadow of the moon Mimas and the planet’s magnificent ring system. In the image of Uranus,
G. Jupiter, as well as all of the Jovian planets, has rings. However, its rings are not as large or as visible as those of Saturn. The rings were not discovered until spacecraft were able to image the planet from behind so as to see the rings in relief.
LOCATION: planets that form in denser parts of the solar nebula (closer to the proto Sun in the center) form their cores first. TIMING: the planet that gets biggest fastest captures the most hydrogen & helium gas.
Describe the cloud formation and atmospheric structure of the gas giants. Characterize the giant planets’ wind and weather patterns. Understand the scale and longevity of storms on the giant planets. The atmospheres of the jovian planets are the parts we can observe or measure directly.
The order in which they condense with increasing depth varies from planet to planet. The altitude at which these condense will increase with increasing saturation vapor pressure, decrease with increasing abundance, and increase with increasing temperature.
