The Giant Planets - Jupiter, Saturn, Uranus, and Neptune - are fluid objects. They have no solid surfaces because the light elements constituting them do not condense at solar-system temperatures. Instead, their deep atmospheres grade downward until the distinction between gas and liquid becomes meaningless. The preceding chapter delved into the hot, dark interiors of the Jovian planets. This one focuses on their atmospheres, especially the observable layers from the base of the clouds to the edge of space. These veneers are only a few hundred kilometers thick, less than one percent of each planet's radius, but they exhibit an incredible variety of dynamic phenomena
Long path, low temperature, moderate resolution spectra of methane and ammonia, broadened by hydroge...
Despite major differences in the solar and internal energy inputs, the atmospheres of the four Jovia...
We examine the properties of exoplanetary atmospheres using state-of-the-art retrieval methods and t...
In seeking to understand the formation of the giant planets and the origin of their atmospheres, the...
Uranus and Neptune are the last unexplored planets of the Solar System. I show that they hold crucia...
All nine planets, four moons, and most comets have atmospheres. These gaseous envelopes are remarka...
All nine planets, four moons, and most comets have atmospheres. These gaseous envelopes are remarka...
The gas giants (Jupiter and Saturn) and icy giants (Uranus and Neptune) are fluid planets with atmos...
Giant planet atmospheres provided many of the surprises and remarkable discoveries of planetary expl...
Giant planet atmospheres provided many of the surprises and remarkable discoveries of planetary expl...
This resource includes pictures, diagrams and brief details about the four outer giant planets: Jupi...
Giant planet atmospheres provided many of the surprises and remarkable discoveries of planetary expl...
The observed properties of giant planets, models of their evolution and observations of pro-toplanet...
The giant planets of the outer solar system - Jupiter, Saturn, Uranus, and Neptune - were formed in ...
Spacecraft and groundbased observations of the atmospheres of solar system objects have provided a d...
Long path, low temperature, moderate resolution spectra of methane and ammonia, broadened by hydroge...
Despite major differences in the solar and internal energy inputs, the atmospheres of the four Jovia...
We examine the properties of exoplanetary atmospheres using state-of-the-art retrieval methods and t...
In seeking to understand the formation of the giant planets and the origin of their atmospheres, the...
Uranus and Neptune are the last unexplored planets of the Solar System. I show that they hold crucia...
All nine planets, four moons, and most comets have atmospheres. These gaseous envelopes are remarka...
All nine planets, four moons, and most comets have atmospheres. These gaseous envelopes are remarka...
The gas giants (Jupiter and Saturn) and icy giants (Uranus and Neptune) are fluid planets with atmos...
Giant planet atmospheres provided many of the surprises and remarkable discoveries of planetary expl...
Giant planet atmospheres provided many of the surprises and remarkable discoveries of planetary expl...
This resource includes pictures, diagrams and brief details about the four outer giant planets: Jupi...
Giant planet atmospheres provided many of the surprises and remarkable discoveries of planetary expl...
The observed properties of giant planets, models of their evolution and observations of pro-toplanet...
The giant planets of the outer solar system - Jupiter, Saturn, Uranus, and Neptune - were formed in ...
Spacecraft and groundbased observations of the atmospheres of solar system objects have provided a d...
Long path, low temperature, moderate resolution spectra of methane and ammonia, broadened by hydroge...
Despite major differences in the solar and internal energy inputs, the atmospheres of the four Jovia...
We examine the properties of exoplanetary atmospheres using state-of-the-art retrieval methods and t...