Gr.10_Chem_PPT_Ch.7_L.3_Bohr's theory of hydrogen atom (1)
Chapter Overview
Title: Atomic Structure and Periodicity
Authors: Jason Overby, Raymond Chang
Edition: Fourteenth Edition (Mc Graw Hill)
Essential Questions
Bohr model of hydrogen atom
Can we determine the exact location of an electron? Why or why not?
Definitions: orbital, electron configuration, shielding, Aufbau principle
Learning Objectives
Understand Bohr model and its explanation of atomic emission spectra in hydrogen.
Atomic Models Timeline
Understanding electron locations involves indirect methods since inner structures are not visible directly.
Wave-Particle Duality of Light
Light exhibits properties as both wave and particle (photon).
Key Concepts:
Wavelength
Frequency
Quantum energy carried by photons
Wave Properties
Characteristics of waves:
Wavelength, frequency, amplitude
Speed (c) relationship: c = frequency × wavelength
Inverse relationship between wavelength and frequency.
Calculating Frequency
Example: Calculate frequency for 686 nm wavelength.
Electromagnetic Radiation Categorization
Categorize radiation based on wavelength:
Ultraviolet, X-rays, Infrared, Microwave, Radio waves, etc.
Photoelectric Effect
Electrons are emitted from metal when illuminated by light.
Photon: particle of light with energy proportional to frequency.
Photonic Energy Formula
Energy of photon: ( E_{photon} = hν )
Where: ( h = 6.626 x 10^{-34} J.s )
Historical Perspective on Emission Spectrum
Newton’s work in the 17th century discovered sunlight's color components.
Spectrum: observable band of colors from light refraction.
Emission: production and release of light.
Characteristics of Emission Spectra
Types of spectra:
Continuous spectrum: all visible light wavelengths.
Line spectra: specific visible light wavelengths.
Emission spectra vary for different substances.
Emission Spectrum of Hydrogen Atom
Energy transition leads to electron jumps between energy states: ground state and excited state.
Emission of light (photons) occurs when electrons return to lower energy levels.
Characteristics of Energy Levels
Ground state (n=1): lowest, stable energy.
Excited states (n>1): higher energy, unstable.
Emission spectrum provides unique identification for each element.
Energy Transition Formula
Energy of photon emitted during electron transition: ( n_{i} \rightarrow n_{f} )
Use Rydberg constant ( R_H = 2.18x10^{-18} ).
Review Questions
Energy Levels: Distinguish ground state vs. excited state.
Emission Spectra: Define and differentiate line from continuous spectra.
Bohr's Theory: Explain hydrogen atom emissions and differences from classical physics principles.