The Ideal Gas Equation and Density
To determine which graph incorrectly represents the behavior of an ideal gas, we must first establish a mathematical relationship between density (d), pressure (p), and temperature (T). We begin our journey with the fundamental equation of state for an ideal gas:
Here, p is the pressure, V is the volume, n is the number of moles, R is the universal gas constant, and T is the absolute temperature.
Since the question asks us to analyze density, we need to introduce mass into our equation. We know that the number of moles n is equal to the given mass w divided by the molar mass M (n=Mw). Substituting this into the ideal gas equation gives:
Deriving the Master Equation
Density (d) is defined as mass per unit volume (d=Vw). To bring density into our equation, we can rearrange the terms to group w and V together:
Replacing Vw with d, we get:
Now, let's isolate density (d) to make it the subject of our formula. By cross-multiplying, we arrive at our master equation:
This elegant equation is the key to unlocking the behavior of the gas under various conditions. Let's use it to analyze each graph one by one.
Analyzing the Graphs
1. Density vs. Temperature (d vs T)
If we keep the pressure (p) constant for a specific gas (constant M), the term RpM becomes a constant. Our master equation simplifies to:
This shows that density is inversely proportional to temperature. Mathematically, an equation of the form y=xk represents a rectangular hyperbola. Graph (I) correctly depicts this hyperbolic curve. However, Graph (II) shows a straight line passing through the origin, implying d∝T. This would mean heating a gas makes it denser at constant pressure, which physically violates Charles's Law. Therefore, Graph (II) is incorrect.
2. Density vs. Inverse Temperature (d vs 1/T)
What happens if we plot density against T1? Let's rewrite our master equation slightly:
If we treat T1 as our independent variable (like x on the x-axis), the equation takes the form y=mx, where the slope m=RpM. This is the equation of a straight line passing through the origin. Graph (III) perfectly illustrates this linear relationship.
3. Density vs. Pressure (d vs p)
Finally, let's examine the relationship between density and pressure at a constant temperature (T). If T is constant, the entire term RTM becomes a constant. Our equation becomes:
This indicates that density is directly proportional to pressure (d∝p). As you compress a gas, its density increases linearly. This relationship is represented by a straight line passing through the origin, which perfectly matches Graph (IV).
Conclusion
By systematically deriving the density formula from the ideal gas law, we have verified that Graphs (I), (III), and (IV) are physically and mathematically sound. Graph (II), which incorrectly suggests a direct proportionality between density and temperature, is the flawed representation. Thus, Graph (II) is our final answer.