The Mechanical Universe
“The Mechanical Universe” is a critically-acclaimed series of 52 thirty-minute videos covering the basic topics of an introductory university physics course
The Mechanical Universe…and Beyond is a critically-acclaimed series of 52 thirty-minute videotape programs covering the basic topics of an introductory university physics course. The series was originally produced as a broadcast telecourse by the California Institute of Technology and Intelecom, Inc. with program funding from the Annenberg/CPB Project.
Each program in the series opens and closes with Caltech Professor David Goodstein providing philosophical, historical and often humorous insight into the subject at hand while lecturing to his freshman physics class. The Mechanical Universe contains hundreds of computer animation segments, created by Dr. James F. Blinn, as the primary tool of instruction. Dynamic location footage and historical re-creations are also used to stress the fact that science is a human endeavor.
Upon completion of the broadcast telecourse, Professor Richard Olenick, Associate Project Director, received funding from the National Science Foundation to produce a seven-hour High School Adaptation suitable for high school physics students. The Mechanical Universe has been translated into nine languages, and a Spanish language version of the High School Adaptation has just been completed.
The series has been broadcast as a telecourse over the PBS television network and can still be seen on many PBS stations. Available on consumer VHS videocassette and laserdisc, and accompanied by textbooks, The Mechanical Universe is arguably the most successful attempt to date to use video technology in the presentation of rigorous physics instruction.
The Mechanical Universe is based on the physics course developed by Dr. David Goodstein at the California Institute of Technology. It was one of twelve projects initially selected for funding by the Annenberg/CPB Project. Course development began with the creation of a set of phantom lectures for the 52 lessons, covering the scientific revolution begun by Copernicus through to current quantum theory. The project was a joint production of Caltech and Intelecom, the largest college television consortia in the United States. The production team included distinguished scientists, video industry professionals, and gifted educators all working in collaboration.
To ensure the highest degree of academic and technical quality, a series of checks and balances was built into the development process. Each program underwent rigorous evaluation by an academic team and a production team, as well as an Oversight Committee, a Local Advisory Committee of educators and a National Advisory Committee comprised of distinguished professionals in film, science, education, and national affairs.
The Mechanical Universe…and Beyond was designed to cover the typical curriculum of a university freshman physics course. As an aid in viewing the topics and subject matter found in the 52 programs, one version of the Table of Contents is presented below.
The Mechanical Universe
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Episode number |
Title |
Directed by |
Written by |
Episode via |
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1 |
“Introduction” |
Peter F. Buffa |
Jack Arnold |
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Brief overview of the material in the first 26 episodes. |
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2 |
“The Law of Falling Bodies” |
Peter F. Buffa |
Peter F. Buffa |
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How falling bodies behave and an introduction to the derivative. |
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3 |
“Derivatives” |
Mark Rothschild |
Pamela Kleibrink |
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Review of the mathematical operation the derivative. |
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4 |
“Inertia” |
Peter F. Buffa |
Albert Abrams |
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How Galileo used the law of inertia to answer questions about the stars. |
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5 |
“Vectors” |
Peter F. Buffa |
Deane Rink |
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Vectors not only have a magnitude but also a direction. |
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6 |
“Newton’s Laws” |
Mark Rothschild |
Ronald J. Casden |
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Newton’s first, second and third laws. |
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7 |
“Integration” |
Mark Rothschild |
Seth Hill & Tom M. Apostol |
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Integration and differentiation are inverse operations of each other. |
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8 |
“The Apple and the Moon” |
Peter F. Buffa |
Don Bane |
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An apple falls and the Moon orbits the Earth because of gravity. |
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9 |
“Moving in Circles” |
Mark Rothschild |
Deane Rink |
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A body in uniform circular motion has both constant speed and constant acceleration. |
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10 |
“Fundamental Forces” |
Mark Rothschild |
Don Bane |
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Gravity, electromagnetism, and the strong and weak nuclear forces. |
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11 |
“Gravity, Electricity, Magnetism” |
Peter F. Buffa |
Don Bane |
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How electricity and magnetism relate to the speed of light. |
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12 |
“The Millikan Experiment” |
Mark Rothschild |
Albert Abrams |
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Millikan’s demonstration to accurately measure the charge of an electron. |
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13 |
“Conservation of Energy” |
Mark Rothschild |
Seth Hill |
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Energy cannot be created or destroyed, only transformed. |
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14 |
“Potential Energy” |
Mark Rothschild |
Don Bane |
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Systems that are stable are at their lowest potential energy. |
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15 |
“Conservation of Momentum” |
Peter Robinson |
Jack George Arnold |
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Momentum is conserved when two or more bodies interact. |
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16 |
“Harmonic Motion” |
Mark Rothschild |
Ronald J. Casden |
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Disturbing stable systems will produce simple harmonic motion. |
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17 |
“Resonance” |
Peter F. Buffa |
Ronald J. Casden |
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Resonance is produced when the frequency of a disturbing force comes close to the natural harmonic frequency of a system. |
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18 |
“Waves” |
Peter F. Buffa |
Ronald J. Casden |
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Waves are a series of disturbances that propagate through solids, liquids and gases. |
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19 |
“Angular Momentum” |
Peter F. Buffa |
Jack George Arnold |
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Objects traveling in circles have angular momentum. |
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20 |
“Torques and Gyroscopes” |
Mark Rothschild |
Jack George Arnold |
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A force acting on a spinning object can cause it to precess. |
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21 |
“Kepler’s Three Laws” |
Peter F. Buffa |
Seth Hill |
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Kepler discovered the orbits of the planets are ellipses. |
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22 |
“The Kepler Problem” |
Peter F. Buffa |
Seth Hill |
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Newton proved that an inverse-square law of gravity implies that celestial bodies move in orbits that are conic sections. |
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23 |
“Energy and Eccentricity” |
Peter F. Buffa |
Seth Hill |
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The conservation of energy and angular momentum help determine how eccentric an orbit will be. |
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24 |
“Navigating in Space” |
Peter F. Buffa |
Don Bane |
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The laws that describe planetary motion are used to navigate in space. |
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25 |
“Kepler to Einstein” |
Peter F. Buffa |
Don Bane, David L. Goodstein |
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Albert Einstein used Newton’s and Kepler’s laws to work on his theory of relativity. |
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26 |
“Harmony of the Spheres” |
Peter F. Buffa |
David L. Goodstein |
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Harmonizing music to the orbits of the planets. |
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The Mechanical Universe …and Beyond
|
Episode number |
Title |
Directed by |
Written by |
Episode via |
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27 |
“Beyond the Mechanical Universe” |
uncredited |
Jack Arnold |
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An overview of the subject matter for the latter half of the series. |
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28 |
“Static Electricity” |
Mark Rothschild |
Donald Button |
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Introducing the concept of electric charge. |
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29 |
“The Electric Field” |
uncredited |
Don Button, Jack Arnold |
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Michael Faraday gave science the image of the electric field. |
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30 |
“Capacitance and Potential” |
uncredited |
Graham Berry, Jack Arnold |
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The basics of the capacitor, with a historical emphasis on Benjamin Franklin. |
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31 |
“Voltage, Energy, and Force” |
Mark Rothschild |
Donald Button |
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Furthering the understanding of how electric charges exert forces and do work. |
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32 |
“The Electric Battery” |
uncredited |
Judith R. Goodstein |
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Thanks to Alessandro Volta’s invention of the electric battery, we can have steady electrical current. |
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33 |
“Electric Circuits” |
Mark Rothschild |
Donald Button |
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The “nuts and bolts” of how electrical circuitry was made practical, featuring Wheatstone, Kirchhoff and Ohm. |
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34 |
“Magnetism” |
uncredited |
Donald Button, Jack Arnold |
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William Gilbert found that the Earth itself is a magnet, a discovery built upon by modern science. |
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35 |
“The Magnetic Field” |
Mark Rothschild |
Jack Arnold |
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Electric currents create, and are influenced by, magnetic fields, per the Biot–Savart and Ampère laws. |
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36 |
“Vector Fields and Hydrodynamics” |
Robert Lattanzio |
Donald Button, Jack Arnold |
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Some concepts apply generally to all vector fields and are useful both in electromagnetism and in the study of fluid flow. |
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37 |
“Electromagnetic Induction” |
uncredited |
Jack Arnold |
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A changing magnetic field creates an electric current: electromagnetic induction, demonstrated by Faraday in 1831. |
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38 |
“Alternating Currents” |
Mark Rothschild |
Jack Arnold |
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In order to make the distribution of electric power practical over great distances, transformers are used to change the voltages of alternating currents. |
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39 |
“Maxwell’s Equations” |
Mark Rothschild |
Jack Arnold |
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By finding the missing conceptual piece in the mathematics of electricity and magnetism, Maxwell discovers light is an electromagnetic wave. |
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40 |
“Optics” |
Robert Lattanzio |
Jack Arnold, David Goodstein |
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Understanding light as a wave makes sense of reflection, refraction, and diffraction. |
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41 |
“The Michelson–Morley experiment” |
uncredited |
Don Bane |
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If light is a wave, what is waving? By careful and precise measurement, Michelson and Morley tried to detect the Earth’s motion through this medium, the “luminiferous aether”, and found nothing. |
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42 |
“The Lorentz Transformation” |
uncredited |
Don Button |
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Einstein realized that, if the speed of light is to be the same for all observers, then distances in space and durations of elapsed time must be relative. |
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43 |
“Velocity and Time” |
uncredited |
Jack Arnold, Richard Bellikoff |
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Einstein arrived at the Lorentz transformation from a deeper conceptual understanding, creating a theory full of surprises like the twin paradox. |
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44 |
“Energy, Momentum, and Mass” |
uncredited |
Jack Arnold |
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The conservation of momentum still applies in special relativity, but with new implications. |
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45 |
“Temperature and the Gas Law” |
uncredited |
Jack Arnold |
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The study of thermodynamics begins with gases. |
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46 |
“The Engine of Nature” |
Mark Rothschild |
Graham Berry, David Goodstein |
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An introduction to the Carnot engine, an idealized machine for converting thermal energy into mechanical work. |
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47 |
“Entropy” |
uncredited |
David Goodstein, Jack Arnold |
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Further investigation of Carnot engines leads to the concept of entropy. |
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48 |
“Low Temperatures” |
uncredited |
Judith R. Goodstein |
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Faraday makes chlorine gas into a liquid, kicking off the pursuit of lower and lower temperatures, culminating in the liquification of helium. |
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49 |
“The Atom” |
uncredited |
David Goodstein, Jack Arnold |
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The ancient Greeks introduced the notion that matter is made of atoms. In the early 20th century, spectral lines and the discovery of the atomic nucleus forced the development of new ideas. |
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50 |
“Particles and Waves” |
uncredited |
Donald Button |
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Light, which had been thought to be a wave, was found to act in some circumstances like a stream of particles. This puzzle led to quantum mechanics. |
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51 |
“Atoms to Quarks” |
uncredited |
Donald Button |
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Understanding the wavefunctions that can be assigned to the electron in a hydrogen atom illuminates the shape of the periodic table of the elements. |
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52 |
“The Quantum Mechanical Universe” |
uncredited |
David Goodstein |
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A review of the series. |
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- Fonte: Caltech | The Mechanical Universe





