This drawing shows the relative location of the hazes of Uranus.
Click on image for full size
Uranus' Atmospheric Hazes
Besides methane, Uranus' atmosphere contains more sophisticated atmospheric molecules such as ethane gas, acetylene, and diacetylene. All these molecules form layers of haze at different altitudes high in the upper
stratosphere, as shown in the picture.
Clouds form at a lower altitude in the troposphere.
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The methane cloud deck of Uranus is found low in the troposphere. The methane clouds are the only clouds to be found on Uranus. The location of the clouds is predicted based upon the temperature at which
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The clouds of Uranus, composed of methane crystals, are found very low in the troposphere, and are difficult to distinquish below the smog haz es of the planet's atmosphere. False color is used, in the
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This diagram shows the temperature profile of Uranus' stratosphere. The temperature becomes warmer with height until the stratopause, or "top" of the stratosphere is reached. As shown in the figure, the
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Besides methane, Uranus' atmosphere contains more sophisticated atmospheric molecules such as ethane gas, acetylene, and diacetylene. All these molecules form layers of haze at different altitudes high
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The mesosphere of Uranus is a region of balance between warming and cooling. That essentially means that nothing happens there. Except for diffusion, the atmosphere is still. Upper reaches of the atmosphere,
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As on Earth, the atmosphere of Uranus consists of a troposphere, stratosphere, mesosphere, and thermosphere. The troposphere is the region where the visible clouds are to be found. The stratosphere, as
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On Uranus, as on Jupiter, the winds in the belts and zones blow first in one direction, then in the opposite direction. Wind blows east in a belt, and west in a zone. The clouds rise up in a belt, and
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