16. The surface temperature of Venus is about 1050 K, and the pressure is about 75.0 earthatmospheres. Assuming that these conditions represent a Venusian "STP", what is the"standard" molar volume of a gas on Venus?17. Gaseous iodine IFs can be prepared by the reaction of solid iodine and gaseous fluorine:k (s) + 5 F2 (g) → 2 IFs (g)A 5.00-L flask is charged with 10.0 g of k and 10.0 g of F2, and the reaction proceedsuntil one of the reagents is completely consumed. After the reaction is complete thetemperature in the flask is 125°C. What is the partial pressure of IFs in the flask?6.

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16. The surface temperature of Venus is about 1050 K, and the pressure is about 75.0 earth atmospheres. Assuming that these conditions represent a Venusian "STP", what is the "standard" molar volume of a gas on Venus?

16. The surface temperature of Venus is about 1050 K, and the pressure is about 75.0 earth atmospheres. Assuming that these conditions represent a Venusian "STP", what is the "standard" molar volume of a gas on Venus?

Chemistry

9th Edition

ISBN:9781133611097

Author:Steven S. Zumdahl

Publisher:Steven S. Zumdahl

Chapter5: Gases

Section: Chapter Questions

Problem 152CP: You have an equimolar mixture of the gases SO2 and O2, along with some He, in a container fitted...

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Question

16. The surface temperature of Venus is about 1050 K, and the pressure is about 75.0 earth
atmospheres. Assuming that these conditions represent a Venusian "STP", what is the
"standard" molar volume of a gas on Venus?
17. Gaseous iodine IFs can be prepared by the reaction of solid iodine and gaseous fluorine:
k (s) + 5 F2 (g) → 2 IFs (g)
A 5.00-L flask is charged with 10.0 g of k and 10.0 g of F2, and the reaction proceeds
until one of the reagents is completely consumed. After the reaction is complete the
temperature in the flask is 125°C. What is the partial pressure of IFs in the flask?
6.

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