91Ó°ÊÓ

To understand molecular weight, think of it as the sum of the weights of all the atoms in a molecule. This is crucial for determining the identity of the gas in various conditions. In the exercise, we need to calculate the molecular weight of an ideal gas. We begin with the formula to find moles, which is the usual practice when using the Ideal Gas Law:

• Re-arrange the Ideal Gas Law: \( n = \frac{PV}{RT} \)

By substituting the values provided (pressure \( P = 2 \text{ atm} \), volume \( V = 5.6035 \text{ L} \), temperature \( T = 546 \text{ K} \)), we find the number of moles to be approximately \( 0.248 \text{ mol} \).
After finding the moles, relate it to molecular weight using:
\[ M = \frac{m}{n} \]where \( m \) is the mass of the gas (\( 4 \text{ g} \)). This step involves dividing the mass by the number of moles to find the molecular weight, which for this exercise, is approximately \( 16.13 \text{ g/mol} \).
Choosing the closest option provided, the correct answer is 16.

The amount of substance, in chemistry, is often expressed in terms of moles. A mole is a convenient unit that contains Avogadro's number of entities, which is \( 6.022 \times 10^{23} \) molecules. This aids in simplifying reactions and calculations.
Using the Ideal Gas Law, we connect physical quantities such as pressure, volume, and temperature to derive the number of moles. Specifically, with:

• \( PV = nRT \)
• \( n = \frac{PV}{RT} \)

We substitute known values into the equation to calculate moles \( n \), binding microscopic gas behavior to measurable properties like pressure and volume.
This principle not only applies to this problem but provides a foundation for understanding real-world gas behavior, illustrating how a measure of something unseen, like moles, affects observable characteristics.

The gas constant, denoted as \( R \), is a vital part of the Ideal Gas Law. It bridges the gap between pressure, volume, temperature, and moles. The value of \( R \) can vary based on the units used, but here it is \( 0.0821 \text{ atm} \cdot \text{L} \cdot \text{K}^{-1} \cdot \text{mol}^{-1} \).
\( R \) is crucial because it provides a universal factor that connects experimental conditions to theoretical calculations. It ensures that pressure and volume changes relate systematically to temperature and moles.
The constant remains a cornerstone in not only understanding ideal gases but forming the base for deviations observed in non-ideal gases under real conditions.