Problem 62
Question
Suppose that on another planet the atmosphere consists of \(10 \% \mathrm{Kr}, 40 \% \mathrm{CH}_{4},\) and \(50 \% \mathrm{O}_{2} .\) What is the average molar mass at the surface? What is the average molar mass at an altitude at which all the \(\mathrm{O}_{2}\) is photodissociated?
Step-by-Step Solution
Verified Answer
The average molar mass at the surface of the planet is \(30.796 g/mol\), and the average molar mass at the altitude where all the \(O_{2}\) is photodissociated is \(14.796 g/mol\).
1Step 1: Calculate the surface average molar mass
To calculate the average molar mass at the surface, first find the molar mass of each gas Kr, CH₄, and O₂. Then, multiply these values by their respective volume percentages and sum the results to obtain the average molar mass.
Molar mass of Kr = 83.8 g/mol
Molar mass of CH₄ = 16.04 g/mol
Molar mass of O₂ = 32.00 g/mol
Surface average molar mass = (0.10)(83.8 g/mol) + (0.40)(16.04 g/mol) + (0.50)(32.00 g/mol)
= 8.38 g/mol + 6.416 g/mol + 16.00 g/mol
2Step 2: Add the individual contributions to find the average molar mass at the surface
Sum the contributions from each gas at the surface to find the final average molar mass:
Surface average molar mass = 8.38 g/mol + 6.416 g/mol + 16.00 g/mol
= 30.796 g/mol
3Step 3: Calculate the average molar mass at the altitude where O₂ is photodissociated
Since all O₂ is photodissociated, we only need to consider the contributions from Kr and CH₄. Using the same method as above, calculate the average molar mass without O₂:
No O₂ average molar mass = (0.1)(83.8 g/mol) + (0.4)(16.04 g/mol)
= 8.38 g/mol + 6.416 g/mol
4Step 4: Add the individual contributions to find the average molar mass at the altitude without O₂
Sum the contributions from Kr and CH₄ to find the final average molar mass:
No O₂ average molar mass = 8.38 g/mol + 6.416 g/mol
= 14.796 g/mol
The average molar mass at the surface of the planet is 30.796 g/mol, and the average molar mass at the altitude where all the O₂ is photodissociated is 14.796 g/mol.
Key Concepts
Understanding Atmospheric CompositionMastering Molar Mass CalculationExploring Photodissociation
Understanding Atmospheric Composition
The atmospheric composition of any planet refers to the different gases that make up its atmosphere. On Earth, for example, we have a mix of nitrogen, oxygen, carbon dioxide, and other gases. Understanding the composition is crucial, as it affects the planet's climate, weather, and even the potential for life.
On the hypothetical planet in our exercise, the atmosphere is made up of 10% krypton (Kr), 40% methane (CH₄), and 50% oxygen (O₂). The percentage indicates the proportion each gas contributes to the total volume of the atmosphere.
When analyzing a planet's atmosphere, consider:
On the hypothetical planet in our exercise, the atmosphere is made up of 10% krypton (Kr), 40% methane (CH₄), and 50% oxygen (O₂). The percentage indicates the proportion each gas contributes to the total volume of the atmosphere.
When analyzing a planet's atmosphere, consider:
- The type of gases present and their chemical properties
- The relative percentages of each gas
- How these gases affect processes such as temperature regulation and radiation shielding
Mastering Molar Mass Calculation
Calculating the average molar mass of a gas mixture involves knowing the molar mass of each component and their respective volume percentages. Molar mass is the mass of a given substance (g) divided by the amount of substance (mol), and it’s typically expressed in g/mol.
To find the average molar mass of an atmosphere:
To find the average molar mass of an atmosphere:
- Identify the molar mass of each component gas. For example, krypton's molar mass is 83.8 g/mol, methane's is 16.04 g/mol, and oxygen's is 32.00 g/mol.
- Multiply the molar mass of each gas by its volume fraction in the atmosphere. This gives the contribution of each gas to the average molar mass.
- Add these contributions together to get the total average molar mass.
Exploring Photodissociation
Photodissociation is a process where molecules are broken down into smaller units due to the absorption of photons, particularly from solar radiation. On Earth, photodissociation is a key player in the chemical changes occurring in the stratosphere, affecting the ozone layer.
In the context of the hypothetical planet, all oxygen ( O₂) molecules are photodissociated at a certain altitude. This leads to significant changes in the atmospheric composition and hence its average molar mass. Without oxygen, only krypton and methane contribute to the molar mass.
When calculating the new average molar mass:
In the context of the hypothetical planet, all oxygen ( O₂) molecules are photodissociated at a certain altitude. This leads to significant changes in the atmospheric composition and hence its average molar mass. Without oxygen, only krypton and methane contribute to the molar mass.
When calculating the new average molar mass:
- O₂ is removed from the calculation, so only the remaining gases are considered.
- The contribution of krypton and methane is recalculated to find the new molar mass.
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