Atomic Structure and Electronic Configuration, Lecture notes of Chemistry

This overview covers atomic structure, the electromagnetic spectrum, and electronic configuration. Key concepts include emission spectrums, spectrum types (line and continuous), and electron excitation/emission. Electronic configuration is explained via the aufbau principle, Hund's rule, and Pauli's exclusion principle. Suitable for high school chemistry/physics, it offers clear explanations with diagrams and examples for exam prep. Ionization energy and electron affinity are touched upon, providing a comprehensive introduction to atomic structure and electronic behavior.

Typology: Lecture notes

2023/2024

Available from 11/22/2025

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2. Atomic Structure
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2. Atomic Structure

Electromagnetic Spectrum: The electromagnetic spectrum is the range of frequencies of electromagnetic radiation and their respective wavelengths. As the wavelength decreases, frequency and energy increase. Emission spectrums: An emission spectrum is the pattern of lines formed when light passes through a prism to separate it into the different frequencies. Types of spectrums: Line spectrum: Only sharp, discrete colors Continuous spectrum: All colors Emission spectra are produced when photons are emitted from atoms as excited electrons return to a lower energy level. Process: ● After an electron is stimulated (e.g., by radiation), it becomes excited ● It moves from its original orbit to an outer orbit. The process is also known as absorption ● Then it returns to its original orbit, and releases energy in the form of a photon ● The photon releases its transition from a higher energy level to a lower energy level corresponding to a certain wavelength. ● Emission (line) spectrums are produced by excited atoms as they fall back to a lower energy level and only contain specific colors (wavelengths, frequencies) of visible light

Paschen (IR) lowest^ energy

Balmer (visible) n = 3

n = 2 Lyman^

(UV (^) light) (^) highest energy n= 1 S

It U

n - >^ n2^ - >^ n]

freq

decreases wavelength In emission^ spectrum , (^) photons are^ emitted^ when^ e-go

to lower

energy levels

O

O

emission absorbtin

high amount (^) of energy emitted => shorter

wavelength

·

B &^ D^ are^ Sabsorption

not emission · choice^ blu^ A &^ C n: 1 -^ >^ n^ = 3 shorter (^) radiation tha n = 2 =^ n= 1 => longest wavelength C

s s p s p s d p s d p s f d p s f d p Orbitals: ● No more than two electrons can occupy any one orbital and if two electrons are in the same orbital they must spin in opposite directions (Pauli’s Exclusion Principle) ● Electrons are placed into orbitals of lowest energy first (Aufbau Principle) ● Orbitals of the same sub-level are filled singly first, then doubly. If more than one orbital in a sub-level is available, electrons occupy different orbitals with parallel spins (Hund’s Third Rule). ● There are four main energy levels ● Each main energy level is divided into several sub-levels ● Sub-levels contain a fixed number of orbitals , regions in space where electrons are likely to be found. ● Sub-level is a group of orbitals with particular properties like shape and angular momentum ● Orbitals can take up to 4 different shapes s-orbitals take a spherical shape p-orbitals resemble a “dumbbell” shape ● Every orbital can hold up to two electrons maximum: ○ s: 1 orbital, 2 electrons ○ p: 3 orbitals, 6 electrons ○ d: 5 orbitals: 10 electrons ○ f: 7 orbitals, 14 electrons ·

ven

affinity (AE)^

is (^) exothermic

(negative values)^

because energy is (^) released as e-^ is^ added · lonization energy (IE) is^ encothermic^ (positive values)^ because energy is absorbed as^ e-^ is^ removed.