Chapter 12: Problem 55
There is free rotation about the carbon-carbon \(\sigma\) -bond in ethane. This means that the energy difference between the staggered and eclipsed conformers is: (a) \(3 \mathrm{~kJ} \mathrm{~mol}^{-1}\) (b) \(23 \mathrm{~kJ} \mathrm{~mol}^{-1}\) (c) \(13 \mathrm{~kJ} \mathrm{~mol}^{-1}\) (d) \(17 \mathrm{~kJ} \mathrm{~mol}^{-1}\)
Short Answer
Step by step solution
Understand Ethane's Bond Rotation
Compare Staggered and Eclipsed Conformers
Know the Energy Difference
Identify the Correct Energy Difference
Select the Closest Answer
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Key Concepts
These are the key concepts you need to understand to accurately answer the question.
Sigma Bond Rotation
Conformers result from the angle between hydrogens attached to each carbon. During \(\sigma\)-bond rotation, you can visualize ethane constantly switching through different states or arrangements. This is a key feature of single bonds and a fundamental aspect of molecular dynamics, giving rise to varied chemical and physical properties in molecules.
Staggered and Eclipsed Conformations
The staggered conformation is the most stable arrangement. Here, hydrogen atoms are positioned as far apart from each other as possible, reducing electron cloud repulsions. This spatial arrangement minimizes the energy, making the staggered conformation energetically favorable.
On the other hand, the eclipsed conformation occurs when hydrogens align with one another. Imagine them standing in a straight line behind each other. In this state, the repulsive interactions between adjacent hydrogen atom electron clouds are maximized. As a result, the eclipsed conformation is less stable and possesses higher energy.
Energy Difference in Conformations
The energy difference between these conformers is not just academic—it directly affects molecular behavior and reactions. For ethane, this energy difference is approximately \(12-14\, \text{kJ/mol}\). The staggered form experiences the lowest energy, while the eclipsed state represents a higher energy plateau.
Calculating or experimentally determining these energy differences helps chemists understand the dynamics of molecules. This information is crucial in predicting how molecules will interact, react, and change shape under different conditions.
Bond Rotation Barrier
Even though the \(\sigma\)-bond allows for rotation, it isn't entirely unrestricted. To move from a staggered to an eclipsed state, a molecule must have enough energy to overcome this barrier. The magnitude of this barrier for ethane, around \(12-14\, \text{kJ/mol}\), reflects how much energy you need to surpass these electron repulsions.
Understanding these barriers is essential, as it illustrates the flexibility or rigidity of molecular structures. In simpler terms, it tells us how easily a molecule can twist and turn in response to environmental factors or reactions.