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They are farther from the sun.
The gas giants are composed of hydrogen and helium, which can remain in a gaseous state at extremely low temperatures, even lower than thous found in the atmospheres of the gas giants. In reality, though, most of the volume of the gas giants is not gas. Deep within the atmospheres of these planets the enormous pressure renders the hydrogen and helium into a supercritical state, which is characteristics between those of a liquid and a gas. Even deeper the hydrogen enters an exotic metal-like state. The interiors of the gas giants are very hot.
Gravity, combined with low surface temperatures.
Not all gas giant planets have low temperatures (most exoplanets are hot "jupiters"). In our solar system the relatively low temperature are a result of the distance they are from the Sun.
According to Charles law, the volume of gas decreases with lower temperatures and increases with higher temperatures
They are farther from the sun.
No. The temperature usually increasesgreatlytowards the interiors ofthe gas giants.
The gas giant planets (Jupiter, Saturn, Uranus, and Neptune) are much farther from the Sun than the inner planets, and so receive less solar heating. They are very hot in their interiors, however, due to compression from the large overlying atmosphere.It is difficult to accurately theorize what their mass, size, and composition would be if they were in closer orbits, but they would have higher average temperatures. The second reason for the low average temperature of gas giants is their large diameter, with a greater volume of atmosphere farther from the layers that have higher compression and heat retention. Even for Earth, the majority of the atmosphere (in the higher altitudes) is extremely cold by surface standards.
The gas giants are composed of hydrogen and helium, which can remain in a gaseous state at extremely low temperatures, even lower than thous found in the atmospheres of the gas giants. In reality, though, most of the volume of the gas giants is not gas. Deep within the atmospheres of these planets the enormous pressure renders the hydrogen and helium into a supercritical state, which is characteristics between those of a liquid and a gas. Even deeper the hydrogen enters an exotic metal-like state. The interiors of the gas giants are very hot.
they are farther from the sun
Gravity, combined with low surface temperatures.
The inner planets did not collect gas like the gas giants did because of their closeness to the Sun. The high temperatures allow for rocky, solid surfaces to form.
Because they are further from the sun.
The gas giant planets (Jupiter, Saturn, Uranus, and Neptune) are much farther from the Sun than the inner planets, and so receive less solar heating. They are very hot in their interiors, however, due to compression from the large overlying atmosphere.It is difficult to accurately theorize what their mass, size, and composition would be if they were in closer orbits, but they would have higher average temperatures. The second reason for the low average temperature of gas giants is their large diameter, with a greater volume of atmosphere farther from the layers that have higher compression and heat retention. Even for Earth, the majority of the atmosphere (in the higher altitudes) is extremely cold by surface standards.
Not all gas giant planets have low temperatures (most exoplanets are hot "jupiters"). In our solar system the relatively low temperature are a result of the distance they are from the Sun.
Exhaust Gas Recirculation. A small amount of exhaust gas is fed back into the cylinder to lower combustion temperatures and lower tail pipe emissions.
According to Charles law, the volume of gas decreases with lower temperatures and increases with higher temperatures