Resource Lesson
Famous Discoveries: The Franck-Hertz Experiment
Printer Friendly Version
James Franck and Gustav Hertz received the
1925 Nobel Prize in Physics
for their "discovery of the laws governing the impact of an electron upon an atom."
In their experiments with mercury during 1912-1914, these two scientists confirmed
Bohr's hypothesis
of discrete atomic energy states and the resulting spectral lines atoms radiate. Bohr had suggested that monochromatic light was emitted only when electrons gave up a discreet amount of energy equal to the difference between two energy states. The experimentation of Franck-Hertz showed that the kinetic energy of cathode rays (electrons) could be used to "boost" steady-state orbital electrons to higher energy states. The energy required was documented as a lose of kinetic energy in the electron beam.
Their experimental numerical results were not only in agreement with Bohr's theory but also corresponded to know wavelengths in mercury's spectrum. In their work, they cited the
1908 work of Walter Ritz
which stated that all of an atom's radiated frequencies (spectral lines) were equal to either the sum or the difference of two other emitted frequencies as well as
Philipp Lenard's
1905 Nobel Prize winning work with cathode ray tube design and properties of electron beams.
Energized electrons (cathode rays) were
released from a filament
and sent through a tube filled with low pressure mercury.
Mercury
atoms (atomic number 80) are monatomic with 78 of their electrons closely bound to their nuclei. Only the two outer-most electrons are "free" to interact with the cathode rays. When low-energy electrons (0-4.5 eV) in the cathode rays struck the ground-state Mercury atoms, the collisions appeared to be elastic - that is, the electron bounced off the Mercury atoms with very little loss of energy. This was measured by the fact that the stopping potential almost exactly equaled the original accelerating potential for the electron beam.
Image courtesy of Kansas State University
However, when electrons were accelerated to energies between 5 and 6 eV, the stopping potentially radically changed to only 0.1 to 1.1 eV. The electrons consistently lost 4.9 eV of energy during their collisions with the Mercury atoms. The collisions were no longer elastic, they were now
inelastic
and a high percentage of the original kinetic energy was absorbed as potential energy by the Mercury atoms. They concluded that the Mercury atoms were entering a new "stable state" with the addition of the 4.9 eV of energy transferred from the electrons. Their results confirmed that ground state Mercury atoms could only accept 4.9 eV of energy - no more, no less.
If the voltage between the filament and the grid is increased, the amount of current would increase; but the current would still exhibit consistent "drop-offs" at intervals of 4.9 eV. It is as if the electrons, upon losing some their initial energy upon colliding with one Mercury atom (4.9 eV), are
accelerated by the field
and upon attaining 4.9 eV or more, can once again exchange energy with a subsequent Mercury atom.
Image courtesy of Kyushu University
Upon learning of Bohr's hypothesis, Franck and Hertz tested the radiation from heated Mercury gas and confirmed that there was indeed an emission line corresponding to 4.9 eV which had a frequency of 1.183 x 10
15
hz, corresponding to a wavelength of 254 nm. The kinetic energy lost in collisions between the electrons in the cathode ray and the ground-state Mercury atoms exactly matched the emission spectra of the heated gas.
Bibliography:
Answers.com
- Franck-Hertz Experiment
Hyperphysics
- The Franck-Hertz Experiment
Hyushu University
- 4-3: The Bohr Model of Atoms
Kansas State University
- Visual Quantum Mechanics
Nobelprize.org
- The Nobel Prize in Physics 1905 Presentation Speech
Nobleprize.org
- The Nobel Prize in Physics 1925 Presentation Speech
Space Research Institute
- (Q-3) Atomic Energy Levels
University of California at San Diego
- Experiment 5: The Franck-Hertz Experiment
Related Documents
Lab:
Labs -
A Battering Ram
Labs -
A Photoelectric Effect Analogy
Labs -
Air Track Collisions
Labs -
Ballistic Pendulum
Labs -
Ballistic Pendulum: Muzzle Velocity
Labs -
Basic Particles
Labs -
Bouncing Steel Spheres
Labs -
Collision Pendulum: Muzzle Velocity
Labs -
Conservation of Momentum
Labs -
Conservation of Momentum in Two-Dimensions
Labs -
Experimental Radius
Labs -
Hydrogen Spectrum
Labs -
Hydrogen Spectrum
Labs -
Impulse
Labs -
Inelastic Collision - Velocity of a Softball
Labs -
Mass of an Electron
Labs -
Mass of the Top Quark
Labs -
Mirror Symmetry
Labs -
Quantized Mass
Labs -
Radiation of a Metal Cylinder
Labs -
Rube Goldberg Challenge
Labs -
Spring Carts
Labs -
Using Young's Equation - Wavelength of a Helium-Neon Laser
Labs -
Video LAB: Ball Re-Bounding From a Wall
Labs -
Video Lab: Blowdart Colliding with Cart
Labs -
Video Lab: Cart Push #2 and #3
Labs -
Video Lab: M&M Collides with Pop Can
Labs -
Video Lab: Marble Collides with Ballistic Pendulum
Resource Lesson:
RL -
A Further Look at Impulse
RL -
An Outline: Dual Nature of Light and Matter
RL -
Atomic Models and Spectra
RL -
Derivation of Bohr's Model for the Hydrogen Spectrum
RL -
Energy-Level Diagrams
RL -
Excitation
RL -
Famous Discoveries and Experiments
RL -
Famous Discoveries: Bohr Model
RL -
Famous Discoveries: de Broglie Matter Waves
RL -
Famous Discoveries: The Photoelectric Effect
RL -
Famous Experiments: Davisson-Germer
RL -
Famous Experiments: Michelson-Morley
RL -
Famous Experiments: Millikan's Oil Drop
RL -
Famous Experiments: The Compton Effect
RL -
Famous Experiments: The Discovery of the Neutron
RL -
Linear Momentum
RL -
Momentum and Energy
RL -
Nuclear Reaction
RL -
Springs and Blocks
RL -
Symmetries in Physics
RL -
What is Mass?
REV -
Orbitals
Worksheet:
APP -
Eternally Bohring
APP -
Nuclear Flu
APP -
Puppy Love
APP -
The Jogger
APP -
The Pool Game
APP -
The Raft
APP -
The Science Fair
APP -
What's My Line
CP -
Atomic Nature of Matter
CP -
Atomic Nucleus and Radioactivity
CP -
Balancing Nuclear Equations
CP -
Conservation of Momentum
CP -
Momentum
CP -
Momentum and Energy
CP -
Momentum and Kinetic Energy
CP -
Momentum Practice Problems
CP -
Momentum Systems and Conservation
CP -
Natural Transmutations
CP -
Nuclear Fission and Fusion
CP -
Radioactive Half Life
CP -
The Atom and the Quantum
NT -
Atomic Number
NT -
Beta Decay
NT -
Binding Energy
NT -
Black Holes
NT -
Electrostatic Attraction
NT -
General Relativity
NT -
Helium Balloons
NT -
Hot Springs
NT -
Hydrogen Atom
NT -
Hydrogen Fusion
NT -
Ice Boat
NT -
Momentum
NT -
Nuclear Equations
NT -
Photoelectric Effect
NT -
Radiant Energy
NT -
Radioactive Cookies
NT -
The Ax Handle
NT -
Uranium Decay
NT -
Uranium Fission
RL -
Chapter 3: Electrons
WS -
Advanced Properties of Freely Falling Bodies #1
WS -
Advanced Properties of Freely Falling Bodies #2
WS -
Advanced Properties of Freely Falling Bodies #3
WS -
Atomic Models and Spectra
WS -
Charged Projectiles in Uniform Electric Fields
WS -
Energy Level Diagrams
WS -
Force vs Displacement Graphs
WS -
Parallel Reading - The Atom
WS -
Practice: Momentum and Energy #1
WS -
Practice: Momentum and Energy #2
WS -
Rotational and Reflection Symmetries
WS -
Standard Model: Particles and Forces
TB -
38A: Atomic Physics
TB -
Half-Life Properties
PhysicsLAB
Copyright © 1997-2023
Catharine H. Colwell
All rights reserved.
Application Programmer
Mark Acton