Hot Jupiters are giant gas planets that orbit very close to their stars. They are believed to have migrated inward from their original formation locations due to interactions with the protoplanetary disk or other planets in the system. This migration process could have been caused by gravitational interactions or tidal forces, leading to their current close proximity to their stars.
"The theory was not based on accurate observations" does not describe a scientifically reasonable explanation for why the nebular theory failed to predict the existence of hot Jupiters. The actual reason is that hot Jupiters were not part of the original models due to limitations in our understanding of planet formation and migration processes.
Small & cold.
The exoplanets called "Hot Jupiters."
Many extrasolar planets are called hot-Jupiters because they are gas giants like Jupiter but much closer to their parent stars, leading to high surface temperatures. Their close proximity to the star results in rapid orbital periods and high levels of irradiation, causing them to be hot compared to Jupiter in our solar system.
Planets like HD 189733 b, sometimes called "hot Jupiters" are one of the most common types of planets to be detected, largely because they are the easiest to detect. Such planets likely form at a great distance from their parent stars, but their orbits decay, bringing them extremely close to their stars. Hot Jupiters often slowly lose their atmospheres.
"The theory was not based on accurate observations" does not describe a scientifically reasonable explanation for why the nebular theory failed to predict the existence of hot Jupiters. The actual reason is that hot Jupiters were not part of the original models due to limitations in our understanding of planet formation and migration processes.
Models suggest that the clouds on hot Jupiters could be composed of minerals like corundum and silicates, as well as exotic compounds such as titanium oxide and aluminum oxide. These clouds may form due to strong winds, vertical mixing, and high temperatures in the atmospheres of hot Jupiters.
Small & cold.
The "exoplanets" known as "Hot Jupiters".
The exoplanets called "Hot Jupiters."
Many newly detected extrasolar planets are called hot Jupiters because they are large, gaseous planets with characteristics similar to Jupiter, but they orbit very close to their host star. This proximity to their star causes them to have high surface temperatures, hence the term "hot."
Many extrasolar planets are called hot-Jupiters because they are gas giants like Jupiter but much closer to their parent stars, leading to high surface temperatures. Their close proximity to the star results in rapid orbital periods and high levels of irradiation, causing them to be hot compared to Jupiter in our solar system.
Planets like HD 189733 b, sometimes called "hot Jupiters" are one of the most common types of planets to be detected, largely because they are the easiest to detect. Such planets likely form at a great distance from their parent stars, but their orbits decay, bringing them extremely close to their stars. Hot Jupiters often slowly lose their atmospheres.
The discovery of hot Jupiters has challenged our understanding of planetary formation in our own Solar System. Their presence suggests that the processes that lead to the formation and migration of giant planets may be more complex and varied than previously thought, leading scientists to reevaluate existing models of planetary formation and migration.
Hot Jupiters were among the earliest known exoplanets discovered because they are large gas giants that orbit very close to their parent stars, making them easier to detect using early planet-hunting techniques.
Because of it's hot, boiling weather.
the explanation for this is to d with the latent heat of water.