Is energy emitted or absorbed when the following electronic transitions occur in hydrogen? (a) from \(n=4\) to \(n=2\) , (b) from an orbit of radius 2.12 A to one of radius \(8.46 \hat{A},(\mathbf{c})\) an electron adds to the \(\mathrm{H}^{+}\) ion and ends up in the \(n=3\) shell?

Short Answer

Expert verified
(a) Energy is emitted during the transition from n=4 to n=2. (b) Energy is absorbed during the transition from 2.12 Å to 8.46 Å. (c) Energy is emitted when an electron adds to the H+ ion and ends up in the n=3 shell.

Step by step solution

01

(a) Transition from n=4 to n=2

Here, we need to determine if energy is emitted or absorbed during a transition from n=4 to n=2. First, let's observe their energy levels using the relation mentioned above: \(E_4 = -\cfrac{13.6 \text{ eV}}{4^2} = -0.85 \text{ eV}\) \(E_2 = -\cfrac{13.6 \text{ eV}}{2^2} = -3.40 \text{ eV}\) Since the electron transitions from a higher energy level (n=4) to a lower energy level (n=2), energy is emitted.
02

(b) Transition from 2.12 Å to 8.46 Å

For this case, we have to find the energy levels corresponding to the given radii. The formula to find the radius, r, of the nth orbit in hydrogen is: \(r_n = 0.529n^2 \ Å\) Solving for n for the two given radii, we get: \(n_1^2 = \cfrac{2.12}{0.529} \Rightarrow n_1 = 2\) \(n_2^2 = \cfrac{8.46}{0.529} \Rightarrow n_2 = 4\) Here, an electron transitions from an orbit with a radius of 2.12 Å (n=2) to an orbit with a radius of 8.46 Å (n=4). Since the electron transitions from a lower energy level (n=2) to a higher energy level (n=4), energy is absorbed.
03

(c) An electron adds to the H+ ion and ends up in the n=3 shell

For this situation, we have an electron joining an H+ ion, which is a hydrogen atom without an electron. When the electron joins and ends up in the n=3 shell, it goes from free space, where its energy is approximately 0 eV, to the n=3 orbit in the hydrogen atom. We already know from the analysis that the energy level for n=3 is: \(E_3 = -\cfrac{13.6 \text{ eV}}{3^2} = -1.51 \text{ eV}\) Since the electron transitions from a higher energy level (0 eV) to a lower energy level (n=3), energy is emitted. In summary: (a) Energy is emitted during the transition from n=4 to n=2. (b) Energy is absorbed during the transition from 2.12 Å to 8.46 Å. (c) Energy is emitted when an electron adds to the H+ ion and ends up in the n=3 shell.

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Key Concepts

These are the key concepts you need to understand to accurately answer the question.

Energy Levels in Hydrogen
Among the fascinating aspects of atomic physics are the energy levels in hydrogen, the simplest atom. A hydrogen atom consists of a single electron orbiting a single proton, and although simple, it indeed holds the key to understanding complex atomic structures.

To grasp this concept, picture the atom as a tiny solar system where the electron can only orbit the proton at certain definite distances. These orbits correspond to energy levels, which are analogous to the
Atomic Spectral Lines
Now, let's dive into atomic spectral lines, which are like the atom's unique fingerprint. Each element emits light at specific frequencies resulting in a spectrum when an electron transitions between energy levels in an atom. This spectrum consists of distinct lines at very precise colors or wavelengths.

Why does this happen? The secret lies in the energy difference between levels. When an electron falls from a higher energy state to a lower one, it
Bohr Model of the Hydrogen Atom
To make sense of these electron transitions and energy levels, we turn to the Bohr model of the hydrogen atom. Proposed by Niels Bohr in 1913, this model revolutionized how we visualize the atom. Bohr's work is pivotal as it introduced quantized orbits or energy levels, where electrons can reside free from radiation.

The Bohr model suggests that electrons circle the nucleus in fixed orbits and can jump between these orbits by absorbing or emitting energy

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Most popular questions from this chapter

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