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← Week 5 Master Hub Topic 1.6 Guide
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AP Chemistry Student Binder Companion · Unit 1: Topic 1.6

Print this dedicated study guide and place it in your 3-ring binder under Unit 1: Atomic Structure & Properties. Refer to the worked AP walkthrough models before attempting your homework problems.

Topic 1.6 Dedicated Guide

Photoelectron Spectroscopy (PES)

Experimental Evidence for Subshells, Binding Energy Principles, Relative Intensity & Core Peak Shifts
Course: AP Chemistry Unit: Unit 1 (Atomic Structure & Properties) Instruction: Jeremy Krug Framework Platform: SABIS-CHEMISTRY.COM

1. The Experimental Contradiction of the Bohr Model

In 1913, Niels Bohr modeled electrons orbiting the atomic nucleus in fixed concentric shells ($n = 1, 2, 3\dots$). If the Bohr model had been complete, all electrons belonging to the same principal energy level (for instance, the 8 electrons in shell $n = 2$) would be located at the exact same average distance from the nucleus and have identical energy.

Under that hypothesis, ejecting any electron from the $n = 2$ shell would require the exact same quantity of energy. However, when multielectron atoms like Neon ($1s^2 2s^2 2p^6$) are ionized in a photoelectron spectrometer, electrons in the $n = 2$ shell produce two distinctly different energy peaks: one at $4.68\text{ MJ/mol}$ ($2s$) and one at $2.08\text{ MJ/mol}$ ($2p$).

The Quantum Mechanical Resolution
Electrons in the same principal energy shell do not have identical energies. They are partitioned into subshells ($s, p, d, f$) having differing spatial geometries, radial distributions, and penetration abilities.

2. Physics of the PES Spectrometer: Conservation of Energy

Photoelectron spectroscopy is the direct laboratory application of Albert Einstein's photoelectric effect to isolated, gas-phase atoms:

  1. Monochromatic Photons: High-energy photons of known frequency $\nu$ and energy $E_{\text{photon}} = h\nu$ (typically ultraviolet or X-rays) strike a gas-phase sample.
  2. Photoelectron Ejection: If $E_{\text{photon}} > \text{Binding Energy}$, a bound electron is ejected from the atom.
  3. Conservation of Energy Accounting:
    E_photon = Binding Energy (BE) + Kinetic Energy (KE)
    Binding Energy (BE) = E_photon - KE
  4. Detector Measurement: The spectrometer measures the kinetic energy ($\text{KE}$) of escaping photoelectrons. Since $E_{\text{photon}}$ is precisely calibrated, the binding energy holding each electron to the nucleus is determined directly.
Photoelectric Effect Principle & Electron Ejection
Figure 1.6-1 (Wikimedia Commons): The Physical Basis of PES — Photons of energy $h\nu$ strike bound electrons, transferring energy to overcome the binding energy ($\text{BE}$) and ejecting electrons with kinetic energy ($\text{KE}$).
X-ray Photoelectron Spectroscopy Energy Level Transitions
Figure 1.6-2 (Wikimedia Commons): Core vs. Valence Orbital Transitions in Photoelectron Spectroscopy — Core electrons ($1s$) require high energy X-rays, whereas valence electrons are ejected with lower photon energies.

3. Reading the Spectrum: Jeremy Krug's Backwards Convention

Golden Rule: The x-Axis Runs BACKWARDS!
On every AP Chemistry exam PES spectrum, high binding energy is plotted on the FAR LEFT (closest to the nucleus). Low binding energy is plotted on the FAR RIGHT (outer valence electrons).
Full PES Spectrum of Neon (1s2 2s2 2p6)
Figure 1.6-1 (From AP 1.6 Slide 14): Authentic AP Exam PES Spectrum of Neon ($1s^2 2s^2 2p^6$) — Three distinct peaks with relative peak heights 1 : 1 : 3 ($2e^- : 2e^- : 6e^-$). The $x$-axis runs backwards with highest binding energy ($1s^2$) on the far left.
Hydrogen vs Helium PES Spectra
Figure 1.6-2 (From AP 1.6 Slide 11): Comparing Hydrogen ($1s^1$) vs. Helium ($1s^2$) — Two fundamental PES rules in one glance: Helium holds 2 electrons (peak is twice as tall as H) and has 2 protons (peak is shifted left to higher binding energy, $2.37\text{ MJ/mol}$ vs $1.31\text{ MJ/mol}$).
Binding Energy (MJ/mol) — Runs Backwards (Decreasing →) Relative Number of Electrons 100 10 1.0 0.1 2 e⁻ 6 e⁻ 1s² 2 84.0 2s² 2 4.68 2p⁶ 6 2.08 ⚡ Core Shell (n = 1) ✨ Valence Shell (n = 2)
Figure 1.6-3: Annotated breakdown of neutral Neon ($1s^2 2s^2 2p^6$) peaks showing core vs. valence shell energy gaps.
Spectral Feature Physical Meaning How to Interpret on the AP Exam
Peak Position (x-axis) Binding Energy ($\text{BE}$) Identifies subshell identity ($1s > 2s > 2p > 3s > 3p$). Leftmost peak is ALWAYS $1s$.
Peak Height / Area (y-axis) Relative number of electrons Tells how many electrons occupy that subshell ($s = 2, p = 6, d = 10$).
Sum of Peak Heights Total electron count Equals atomic number ($Z$) for neutral atoms.

4. Comparing Identical Subshells: Nuclear Charge Shifts

A classic AP Chemistry question compares identical subshells across different elements (e.g., the $1s$ peak of Nitrogen vs. Oxygen, or Silicon vs. Sulfur).

Core 1s Shift in Nitrogen vs Oxygen
Figure 1.6-4 (From AP 1.6 Slide 17): Core 1s Shift in Nitrogen vs. Oxygen — Oxygen ($Z = 8$) exerts stronger Coulombic attraction on its 1s electrons than Nitrogen ($Z = 7$), shifting its peak to higher binding energy ($52.6\text{ MJ/mol}$ vs. $39.6\text{ MJ/mol}$).
Binding Energy (MJ/mol) — Decreasing → 60 45 30 Oxygen 1s² (Z = 8) 52.6 Nitrogen 1s² (Z = 7) 39.6 Shifted Left (Higher BE) due to +1 proton
Figure 1.6-B: Comparison of 1s core peaks for Nitrogen ($Z = 7$) and Oxygen ($Z = 8$). Oxygen's greater nuclear charge pulls 1s electrons tighter.
AP Exam Trap: Citing Shielding for Core Electrons
Do NOT claim that Oxygen's $1s$ peak has greater binding energy because of "less shielding." Both Nitrogen and Oxygen have zero shielding inside the $1s$ subshell! The shift is caused purely by greater nuclear charge ($Z$) exerting stronger Coulombic attraction ($F \propto \frac{q_1 q_2}{r^2}$).

5. Step-by-Step Worked AP Exam Walkthrough Models

Model 1: Deducing Unknown Element from a PES Spectrum AP Exam FRQ / MCQ

Problem Statement: A photoelectron spectrum for a neutral mystery element exhibits 4 peaks with the following characteristics:

  • Peak 1: $104\text{ MJ/mol}$ (relative height = 2)
  • Peak 2: $6.84\text{ MJ/mol}$ (relative height = 2)
  • Peak 3: $3.67\text{ MJ/mol}$ (relative height = 6)
  • Peak 4: $0.50\text{ MJ/mol}$ (relative height = 1)

Identify the element, write its complete ground-state electron configuration, and identify which peak corresponds to valence electrons.

Step-by-Step Solution:
  1. Identify subshells from left to right (highest to lowest energy):
    • Peak 1 ($104\text{ MJ/mol}$, height 2) = $1s^2$
    • Peak 2 ($6.84\text{ MJ/mol}$, height 2) = $2s^2$
    • Peak 3 ($3.67\text{ MJ/mol}$, height 6) = $2p^6$
    • Peak 4 ($0.50\text{ MJ/mol}$, height 1) = $3s^1$
  2. Total electron count: $2 + 2 + 6 + 1 = 11$ electrons.
  3. Element Identity: Neutral element with 11 protons/electrons is Sodium ($\text{Na}$).
  4. Valence Peak: Peak 4 ($3s^1$, $0.50\text{ MJ/mol}$) represents the outermost valence electron. It has the lowest binding energy because it is farthest from the nucleus and shielded by 10 core electrons.
Model 2: Explaining Core Peak Shifts (Sulfur vs. Silicon) AP Free Response Model

Problem Statement: The $1s$ peak of Sulfur appears at $239\text{ MJ/mol}$, while the $1s$ peak of Silicon appears at $178\text{ MJ/mol}$. Justify this experimental observation using atomic structure and Coulomb's Law.

Model AP Explanation (Full Credit Protocol):

"Both Sulfur ($Z = 16$) and Silicon ($Z = 14$) have two electrons in their 1s subshell. Because these electrons reside in the n = 1 principal shell, the average distance (r) between the 1s electrons and the nucleus is approximately equal for both atoms. However, Sulfur possesses 16 protons in its nucleus, compared to only 14 protons in Silicon. According to Coulomb's Law ($F \propto \frac{q_1 q_2}{r^2}$), the greater nuclear charge in Sulfur exerts a stronger electrostatic attraction on the 1s electrons. Consequently, more energy is required to eject a 1s electron from Sulfur, producing a higher binding energy ($239\text{ MJ/mol}$ vs. $178\text{ MJ/mol}$)."

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