21. On the sunlit surface of Venus, the atmospheric pressure is 9.0 3 106Pa, and the temperature is 740 K. On the earth’s surface the atmosphericpressure is 1.0 3 105 Pa, while the surface temperature can reach 320 K.These data imply that Venus has a “thicker” atmosphere at its surfacethan does the earth, which means that the number of molecules per unitvolume (N/V) is greater on the surface of Venus than on the earth. Findthe ratio (N/V)Venus/(N/V)Earth.
21. On the sunlit surface of Venus, the atmospheric pressure is 9.0 3 106Pa, and the temperature is 740 K. On the earth’s surface the atmosphericpressure is 1.0 3 105 Pa, while the surface temperature can reach 320 K.These data imply that Venus has a “thicker” atmosphere at its surfacethan does the earth, which means that the number of molecules per unitvolume (N/V) is greater on the surface of Venus than on the earth. Findthe ratio (N/V)Venus/(N/V)Earth.
College Physics
10th Edition
ISBN:9781285737027
Author:Raymond A. Serway, Chris Vuille
Publisher:Raymond A. Serway, Chris Vuille
Chapter10: Thermal Physics
Section: Chapter Questions
Problem 9WUE: Suppose 26.0 g of neon gas are stored in a tank at a temperature of 152C. (a) What is the...
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21. On the sunlit surface of Venus, the atmospheric pressure is 9.0 3 106
Pa, and the temperature is 740 K. On the earth’s surface the atmospheric
pressure is 1.0 3 105 Pa, while the surface temperature can reach 320 K.
These data imply that Venus has a “thicker” atmosphere at its surface
than does the earth, which means that the number of molecules per unit
volume (N/V) is greater on the surface of Venus than on the earth. Find
the ratio (N/V)Venus/(N/V)Earth.
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