The Cloud Structure of Venus Can Best Be Described as
Are confined to a narrow layer about 60 km above. These are formed by the very rapid photooxidation of carbonyl sulfide in the upper atmosphere. Life Free Full Text The Case Or Not For Life In The Venusian Clouds Html The cloud structure in the atmosphere of Venus can be described as. . Surface temperatures on Venus are about 900 degrees Fahrenheit 475 degrees Celsius hot. The region in which the atmospheric temperature decreases with altitude. The clouds are more opaque near the equator giving Venus a dark band in Akatsuki IR2 images and more transparent lighter toward the poles. The atmosphere extends to about 250 km above the surface. This altitude difference seems to be one of the main responsible factors in the formation of the so-called cold collar. Venus is closer to the Sun so it gets more intense sunlight Planets cloud-over is highly reflective reflecting 60 of the suns light As seen from Earth the. ...
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