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101526 L2 Chemistry 221 Video Lecture Part I

Michael Russell · 50:10 · Watch on YouTube

101526 L2 Chemistry 221 Video Lecture Part I Watch on YouTube →

Overview

Michael Russell connects photon energy and matter waves to the quantum-number rules used to describe atomic orbitals, then applies those rules to electron configurations. The lesson works through a 182.3 kJ/mol photon transition, de Broglie wavelength calculations, orbital nodes, and configurations for chlorine and tin, including noble-gas notation.

Key takeaways

Chapters

0:00 Earthquake Drill Instructions and Photon Wavelength Problem
6:08 Convert 182.3 kJ/mol into Photon Wavelength
9:21 De Broglie Wavelength of an Electron
17:37 Identify an Invalid Set of Quantum Numbers
19:09 Rules for n, l, mₗ, and mₛ
22:25 Translate Quantum Numbers into 3p Orbital Notation
25:26 Calculate Spherical and Planar Orbital Nodes
31:16 Set Up Chlorine's Electron Configuration
34:39 Build Chlorine's Configuration with Aufbau and Noble-Gas Notation
40:41 Determine Tin's Configuration from Krypton
46:26 Class Ends with the Earthquake Drill Cue

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