Chapter 17: Problem 2
According to the ideal-gas law, what should be the volume of a gas at absolute zero? Why is this result absurd?
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Chapter 17: Problem 2
According to the ideal-gas law, what should be the volume of a gas at absolute zero? Why is this result absurd?
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The average speed of the molecules in a gas increases with increasing temperature. What about the average velocity?
At high gas densities, the van der Waals equation modifies the ideal-gas law to account for nonzero molecular volume and for the van der Waals force that we discussed in Section \(17.1 .\) The van der Waals equation is $$\left(p+\frac{n^{2} a}{V^{2}}\right)(V-n b)=n R T$$ where \(a\) and \(b\) are constants that depend on the particular gas. For nitrogen \(\left(\mathrm{N}_{2}\right), a=0.14 \mathrm{Pa} \cdot \mathrm{m}^{6} / \mathrm{mol}^{2}\) and \(b=3.91 \times 10^{-5} \mathrm{m}^{3} / \mathrm{mol}\) For 1.000 mol of \(\mathrm{N}_{2}\) at 10.00 atm pressure, confined to a volume of \(2.000 \mathrm{L},\) find the temperatures predicted (a) by the ideal-gas law and (b) by the van der Waals equation.
A helium balloon occupies \(8.0 \mathrm{L}\) at \(20^{\circ} \mathrm{C}\) and 1.0 -atm pressure. The balloon rises to an altitude where the air pressure is 0.65 atm and the temperature is \(-10^{\circ} \mathrm{C}\). What's its volume when it reaches equilibrium at the new altitude?
The atmospheres of relatively low-mass planets like Earth don't contain much hydrogen (H \(_{2}\) ), while more massive planets like Jupiter have considerable atmospheric hydrogen. What factors might account for the difference?
(a) If 2.0 mol of an ideal gas are initially at temperature \(250 \mathrm{K}\) and pressure 1.5 atm, what's the gas volume? (b) The pressure is now increased to 4.0 atm, and the gas volume drops to half its initial value. What's the new temperature?
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