Question

Difficulty: HardGas Laws and the Ideal Gas Equation

A rigid gas vessel sealed on a meteorological satellite initially contains a fixed volume of an ideal gas at a pressure of 1.50×105 Pa1.50 \times 10^5\text{ Pa} and a temperature of 27∘C27^\circ\text{C}. During an orbital maneuver, solar radiation heats the vessel to 327∘C327^\circ\text{C}, while a small vent valve simultaneously allows 20%20\% of the gas molecules to escape. Assuming the volume of the vessel remains constant, what is the final pressure of the gas inside the vessel?

  1. 2.40×105 Pa2.40 \times 10^5\text{ Pa}Answer
  2. B
    1.45×106 Pa1.45 \times 10^6\text{ Pa}
  3. C
    3.00×105 Pa3.00 \times 10^5\text{ Pa}
  4. D
    6.00×104 Pa6.00 \times 10^4\text{ Pa}

Answer

2.40×105 Pa2.40 \times 10^5\text{ Pa}
According to the ideal gas law (PV=nRTPV = nRT), when volume is held constant, pressure is directly proportional to both the number of moles of gas present and the absolute temperature in Kelvin (P∝nTP \propto nT). First, convert the initial and final temperatures to Kelvin: T1=27+273=300 KT_1 = 27 + 273 = 300\text{ K} and T2=327+273=600 KT_2 = 327 + 273 = 600\text{ K}. Because 20%20\% of the gas escapes, 80%80\% remains inside the vessel, so n2=0.80n1n_2 = 0.80n_1. Calculating final pressure yields P2=P1×(n2/n1)×(T2/T1)=1.50×105×0.80×(600/300)=2.40×105 PaP_2 = P_1 \times (n_2/n_1) \times (T_2/T_1) = 1.50 \times 10^5 \times 0.80 \times (600/300) = 2.40 \times 10^5\text{ Pa}.

Step-by-Step Solution

1
Convert all given temperatures from degrees Celsius to absolute temperature in Kelvin.
T1=27+273.15=300 KT_1 = 27 + 273.15 = 300\text{ K}, T2=327+273.15=600 KT_2 = 327 + 273.15 = 600\text{ K}
Gas laws and the ideal gas equation require absolute temperature in Kelvin.
2
Determine the fraction of gas remaining in the rigid vessel.
If 20%20\% escapes, remaining fraction n2=(1−0.20)n1=0.80n1n_2 = (1 - 0.20)n_1 = 0.80n_1
Pressure depends on the quantity of gas remaining inside the fixed volume.
3
Apply the ideal gas equation PV=nRTPV = nRT for constant volume VV.
P2=P1×(n2n1)×(T2T1)P_2 = P_1 \times \left(\frac{n_2}{n_1}\right) \times \left(\frac{T_2}{T_1}\right)
Since volume is constant, pressure is directly proportional to the product of amount of gas and absolute temperature.
4
Substitute known values to compute the final pressure P2P_2.
P2=(1.50×105 Pa)×0.80×(600 K300 K)=2.40×105 PaP_2 = (1.50 \times 10^5\text{ Pa}) \times 0.80 \times \left(\frac{600\text{ K}}{300\text{ K}}\right) = 2.40 \times 10^5\text{ Pa}
Multiplying the initial pressure by the mole fraction ratio and temperature ratio gives the final gas pressure.

Key Concept

Ideal Gas Equation and Combined Gas Behavior
Estimated Time:2m 0s
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