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Mechanical Universe - and Beyond. (Programs 21 through 26)

https://did.cit.jmu.edu/default.aspx?direct=image&id=31&res=acpb0131.xml
https://did.cit.jmu.edu/default.aspx?direct=image&id=31&res=acpb0132.xml
https://did.cit.jmu.edu/default.aspx?direct=image&id=31&res=acpb0133.xml
https://did.cit.jmu.edu/default.aspx?direct=image&id=31&res=acpb0134.xml
https://did.cit.jmu.edu/default.aspx?direct=image&id=31&res=acpb0135.xml
https://did.cit.jmu.edu/default.aspx?direct=image&id=31&res=acpb0136.xml

DVD 1481

Program 21 deals with Kepler's three laws which described the motion of heavenly bodies with unprecedented accuracy. Also discusses the relationship between these laws and conic sections first identified by ancient Greek mathematicians. Program 22 deals with what is known as Kepler's problem, the deduction of all three of Kepler's laws from Newton's universal law of gravitation. Program 23 describes the orbit of all heavenly bodies in terms of the laws of conservation of energy and angular momentum. Program 24 discusses how the amount of energy needed to voyage to other planets can be minimized by using the same principles that guide planets around the solar system. Program 25 explains why natural occurrences such as the ebb and flow of tides are a consequence of the law of gravity and this explanation leads to Einstein's general theory of relativity and black holes. Program 26 looks back at material covered in earlier programs. Uses computer animation sequences, historical reenactments, and close-up photography of experiments.

What is Music?

http://did.cit.jmu.edu/default.aspx?direct=image&id=31&res=ffh02310.xml

AE5.F55 Internet

This program examines sound-waves: why some sounds are musical and others just noise, and the relationship of regularity or irregularity of vibration to the perception of musicality, as well as such non-scientific questions as the cultural content of musical perception.

Essence of an Instrument

http://did.cit.jmu.edu/default.aspx?direct=image&id=31&res=ffh02311.xml

AE5.F55 Internet

Program analyzes the essential features required in any instrument if a usable musical sound is to be produced. Program examines how energy can be provided, how sound can be amplified, how amplification changes the quality of sound, and the consequences for music produced by synthesizers and computers.

Science, Strings, and Symphonies

http://did.cit.jmu.edu/default.aspx?direct=image&id=31&res=ffh02312.xml

AE5.F55 Internet

Two groups of instruments use strings as the primary source of sound: those in which plucking set the strings in vibration, and the bowed strings. This program shows how the demand for more powerful sounds was met, and examines the instruments of Stradivari to determine what science can and cannot reveal about their magic. It also examines the ways in which scientific methods complement the skill of craftsmen in making instruments.

Technology, Trumpets and Tunes

http://did.cit.jmu.edu/default.aspx?direct=image&id=31&res=ffh02313.xml

AE5.F55 Internet

Despite its title, this program actually covers all the wind instruments, including the pipe organ. It considers the way in which the technology of making instruments has affected the course of musical development, particularly the development of valves for trumpets and Boehm's system of woodwind keys. The program examines the subject of vibrations in tubes, the role of finger holes, and the components of tone quality. It concludes by putting a camera inside a large church organ to show what happens inside this marvelous combination of thousands of pipes, hundreds of yards of pneumatic tubing or electric cables, and countless valves or relays in response to the movements of the organist's hands and feet.

Scales, Synthesizers and Samplers

http://did.cit.jmu.edu/default.aspx?direct=image&id=31&res=ffh02314.xml

AE5.F55

This program covers such problems as the production of varying degrees of loudness on harpsichords and spinets, the mechanical engineering of the modern piano, the origin of scales, and the inability of keyboard instruments to produce scales in all keys exactly in tune. Synthesizers demonstrate both the problem and its solution. The progression is from electronic organs to analogue synthesizers, from purely electronic oscillations to the addition, subtraction, multiplication, mixing, and performance of additional functions that comprise the complex sounds of music. The program also looks at digital sound and musique concrète, using the BBC Radiophonic Workshop to answer some of the questions about the partnership between science and music.

Mechanical Universe - and Beyond. (Parts 1 through 4)

https://did.cit.jmu.edu/default.aspx?direct=image&id=31&res=acpb0111.xml
https://did.cit.jmu.edu/default.aspx?direct=image&id=31&res=acpb0112.xml
https://did.cit.jmu.edu/default.aspx?direct=image&id=31&res=acpb0113.xml
https://did.cit.jmu.edu/default.aspx?direct=image&id=31&res=acpb0114.xml

DVD 1476

Program 1 introduces revolutionary ideas and heroes from Copernicus to Newton and links the physics of the heavens and the earth. Program 2 covers Galileo's experiments which proved that all bodies fall with the same constant acceleration. Program 3 deals with the function of mathematics in physical science and the derivative as a practical tool. Program 4 deals with Galileo's efforts to answer questions about the nature of universe, the development of his law of inertia, and the risks that he took in challenging accepted knowledge of the period. Uses computer animation sequences, historical reenactments, and close-up photography of experiments.

Mechanical Universe - and Beyond. (Parts 5 through 8)

https://did.cit.jmu.edu/default.aspx?direct=image&id=31&res=acpb0115.xml
https://did.cit.jmu.edu/default.aspx?direct=image&id=31&res=acpb0116.xml
https://did.cit.jmu.edu/default.aspx?direct=image&id=31&res=acpb0117.xml
https://did.cit.jmu.edu/default.aspx?direct=image&id=31&res=acpb0118.xml

DVD 1477

Program 5 deals with the issues addressed by physics: why, how much, where, and which way. Program 6 covers Newton's contribution to the laws of force, mass, and acceleration. Program 7 deals with Newton's and Leibniz conclusion that differentiation and integration are inverse processes. Program 8 covers Newton's discovery that gravity describes the force between any two particles in the universe. Uses computer animation sequences, historical reenactments, and close-up photography of experiments.

Mechanical Universe - and Beyond. (Parts 13 through 16)

https://did.cit.jmu.edu/default.aspx?direct=image&id=31&res=acpb0123.xml
https://did.cit.jmu.edu/default.aspx?direct=image&id=31&res=acpb0124.xml
https://did.cit.jmu.edu/default.aspx?direct=image&id=31&res=acpb0125.xml
https://did.cit.jmu.edu/default.aspx?direct=image&id=31&res=acpb0126.xml

DVD 1479

Program 13 deals with the law of physics which states that energy is neither created nor destroyed. Program 14 deals with potential energy and the powerful model that this concept has become for understanding why the world has worked the same way since the beginning of time. Program 15 likens the universe to a perpetual clock and applies the principle of conservation of momentum to explain why the universe continues to operate. The same principle is also applied to an analysis of collisions. Program 16 explains that the restoring force and inertia of any stable mechanical system causes objects to execute simple harmonic motion. Uses computer animation sequences, historical reenactments, and close-up photography of experiments.

Physics and Physiology of Sports

http://did.cit.jmu.edu/default.aspx?direct=image&id=31&res=ffh05564.xml

AE5.F55 Internet

When we engage in sports activity, we are usually not aware of the scientific way in which the activity combines the principles of physics and physiology. This program describes the principles governing the following sports activities: scuba diving, flying, sailing, and gymnastics. Content ranges from nitrogen bubbles and the "bends" through the Bernoulli principle to semicircular canals, all essential constituents of our sporting activities.

Freeman Dyson

http://did.cit.jmu.edu/default.aspx?direct=image&id=31&res=ffh05082.xml

Videotape no.3854

An interview with Freeman Dyson, a physicist with a particular interest in mathematics, nuclear and astro physics.

Millikan's Oil-Drop Experiment

http://did.cit.jmu.edu/default.aspx?direct=image&id=31&res=ffh01078.xml

AE5.F55 Internet

This program uses a modified version of the Millikan oil-drop apparatus to measure the radius and total charge of oil droplets. Students measure the terminal velocity of an oil drop falling under gravity in order to calculate the radius of the drop. The drop is then charged. An electric field is applied across the Millikan chamber so that the drop is suspended between the plates. The total charge on the drop can be calculated by students from the voltage required to suspend the drop. When this voltage is increased, the drop rises at a terminal velocity. Students can measure this and verify the total charge determined in the static experiment.

Rutherford Scattering of Alpha-Particles, The

http://did.cit.jmu.edu/default.aspx?direct=image&id=31&res=ffh01079.xml

AE5.F55 Internet

This program reproduces the experimental observations which led to the development of the Rutherford model of the atom.

Ionization and Excitation Potential

http://did.cit.jmu.edu/default.aspx?direct=image&id=31&res=ffh01081.xml

AE5.F55 Internet

The energy transfer between accelerated electrons of different energies and atoms when they collide is presented in this program and related to the quantum theory of atomic structure.

Cp/Cv for Helium, Nitrogen and Carbon Dioxide

http://did.cit.jmu.edu/default.aspx?direct=image&id=31&res=ffh01084.xml

AE5.F55 Internet

The ratio of specific heats of gases, Cp/Cv=y, is a signature of the number of atoms in the molecule. In this program, students measure this ratio for mono-, di-, and triatomic gases.

Effect of Pressure on the Thermal Conductivity of a Gas, The

http://did.cit.jmu.edu/default.aspx?direct=image&id=31&res=ffh01085.xml

AE5.F55 Internet

In this program, students measure the thermal conductivity of argon over a wide range of vacuum pressures. Heat is conducted by collisions between molecules. As the pressure of a conducting gas decreases, the number of molecules of gas decreases but the distance between molecules increases, thus keeping the rate of collisions relatively constant.

pV Isotherms of Carbon Dioxide

https://did.cit.jmu.edu/default.aspx?direct=image&id=31&res=ffh01075.xml
https://did.cit.jmu.edu/default.aspx?direct=image&id=31&res=ffh01076.xml

AE5.F55 Internet

Part 1: experiments illustrate changes in the isothermal pressure/volume relationship for a gas under a range of pressures -- Part 2: additional pV isotherms are measured for CO2 both below and above the critical temperature.

Beyond the Mechanical Universe; Static Electricity

https://did.cit.jmu.edu/default.aspx?direct=image&id=31&res=acpb0137.xml
https://did.cit.jmu.edu/default.aspx?direct=image&id=31&res=acpb0138.xml

Videodisc 164-165

Program 27. The world of electricity and magnetism, and 20th-century discovery of relativity and quantum mechanics. Program 28. Eighteenth-century electricians knew how to spark the interest of an audience with the principles of static electricity.

Beyond the Mechanical Universe - Voltage, Energy and Force; Electric Batteries

https://did.cit.jmu.edu/default.aspx?direct=image&id=31&res=acpb0141.xml
https://did.cit.jmu.edu/default.aspx?direct=image&id=31&res=acpb0142.xml

Videodisc 166-167

Program 31. When is electricity dangerous or benign, spectacular or useful? Program 32. Alessandro Volta invents the electric battery using the internal properties of different metals.

Beyond the Mechanical Universe - Electric Circuits; Magnetism

https://did.cit.jmu.edu/default.aspx?direct=image&id=31&res=acpb0143.xml
https://did.cit.jmu.edu/default.aspx?direct=image&id=31&res=acpb0144.xml

Videodisc 168-169

Program 33. The works of Charles Wheatstone, Ohm, and Kirchhoff lead to the design and analysis of how current flows. Program 34. William Gilbert, physician to Queen Elizabeth I of England, discovered that the earth behaves like a giant magnet. Modern scientists have learned even more.

Beyond the Mechanical Universe - Magnetic Field; Vector Fields and Hydrodynamics

https://did.cit.jmu.edu/default.aspx?direct=image&id=31&res=acpb0145.xml
https://did.cit.jmu.edu/default.aspx?direct=image&id=31&res=acpb0146.xml

Videodisc 168-169

Program 35 discusses the relationship between an electric current and the magnetic field it produces, the law of Biot and Sarvart, the force between electric currents, and Ampere's laws. Program 36 discusses the differences between electric fields and magnetic fields and how both can be better understood by analogy to fields of fluid flow.

Beyond the Mechanical Universe - Electromagnetic Induction; Alternating Currents

https://did.cit.jmu.edu/default.aspx?direct=image&id=31&res=acpb0147.xml
https://did.cit.jmu.edu/default.aspx?direct=image&id=31&res=acpb0148.xml

Videodisc 170-171

Program 37. The discovery of electromagnetic induction in 1831 creates an important technological breakthrough in the generation of electric power. Program 38. Electromagnetic induction makes it easy to generate alternating current while transformers make it practical to distribute it over long distances.

Beyond the Mechanical Universe - Maxwell's Equations; Optics

https://did.cit.jmu.edu/default.aspx?direct=image&id=31&res=acpb0149.xml
https://did.cit.jmu.edu/default.aspx?direct=image&id=31&res=acpb0150.xml

Videodisc 170-171

Program 39 discusses the discovery of the displacement current by Maxwell, which completed the electricity and magnetism puzzle. Program 40 discusses the properties of light as the properties of waves, including reflection, refraction and diffraction.

Beyond the Mechanical Universe - The Michelson-Morley Experiment; Lorentz Transformation

https://did.cit.jmu.edu/default.aspx?direct=image&id=31&res=acpb0151.xml
https://did.cit.jmu.edu/default.aspx?direct=image&id=31&res=acpb0152.xml

Videodisc 172-173

Program 41. In 1887, an exquisitely designed measurement of the earth's motion through the ether results in the most brilliant failure in scientific history. Program 42. If the speed of light is to be the same for all observers, then the length of a meter stick, or the rate of a ticking clock, depends on who measures it.

Beyond the Mechanical Universe - Velocity and Time; Energy, Momentum and Mass

https://did.cit.jmu.edu/default.aspx?direct=image&id=31&res=acpb0153.xml
https://did.cit.jmu.edu/default.aspx?direct=image&id=31&res=acpb0154.xml

Videodisc no.172-173

Program 43 discusses the work of Albert Einstein, resulting in the theory of relativity, a wholly new understanding of the meaning of space and time. Program 44 discusses how this new meaning of space and time made it necessary to formulate a new mechanics.

Beyond the Mechanical Universe - Temperature and Gas Laws; Engine of Nature

https://did.cit.jmu.edu/default.aspx?direct=image&id=31&res=acpb0155.xml
https://did.cit.jmu.edu/default.aspx?direct=image&id=31&res=acpb0156.xml

Videodisc no.174-175

Program 45. Hot discoveries about the behavior of gases make the connection between temperature and heat. Program 46. The carnot engine, part one, beginning with simple steam engines.

Beyond the Mechanical Universe - Atoms to Quarks; Quantum Mechanical Universe

https://did.cit.jmu.edu/default.aspx?direct=image&id=31&res=acpb0161.xml
https://did.cit.jmu.edu/default.aspx?direct=image&id=31&res=acpb0162.xml

Videodisc no.176-177

Program 51. Electron waves attracted to the nucleus of an atom help account for the periodic table of elements and ultimately lead to the search for quarks. Program 52. A last look at where we've been and a peek into the future.

Dark Side of the Universe, The

http://did.cit.jmu.edu/default.aspx?direct=image&id=31&res=pbs_saf050.xml

AE5.P37 Internet

New discoveries about dark matter and dark energy have astronomers wondering if ours is but one of an infinity of universes.

Stephen Hawking's Universe: Seeing is Believing - The Big Bang

http://did.cit.jmu.edu/default.aspx?direct=image&id=31&res=pbs_shn000-1.xml

AE5.P37 Internet

Presents the latest advances in cosmological thought, including the mathematics of astronomy, the Big Bang theory of creation, the nature of matter, the discovery and implications of dark matter, quasars and black holes, and the question of how the Big Bang began.

Stephen Hawking's Universe: Black Holes and Beyond - an Answer to Everything

http://did.cit.jmu.edu/default.aspx?direct=image&id=31&res=pbs_shn000-3.xml

AE5.P37 Internet

Black holes and beyond' focuses on Hawking's specialty, black holes. With the invention of radio astronomy over 50 years ago many astronomical discoveries came to light including ultraluminous quasars, wormholes, black holes and singularities. It was discovered that quasars, bizarre objects billions of light years away with a power output greater than all of the stars in our galaxy put together, shine brightly as matter is sucked into a black hole and heats up due to friction. Such discoveries seem to allow for travel over millions of miles of space or even time travel and have even led to SETI--the search for Extra-Terrestrial Intelligence--looking for stray alien communications. 'An answer to everything" asks the question: how did the Big Bang begin? Stephen Hawking is joined by other leading scientists as they try to answer this question. Includes discussions of inflation theory, quantum mechanics, and string theory.

Determination of the Velocity of Light, The

http://did.cit.jmu.edu/default.aspx?direct=image&id=31&res=ffh01072.xml

AE5.F55 Internet

The velocity of light is determined by focusing a deflected laser beam back and forth from a rotating mirror to a fixed mirror and measuring the deflection of the beam's image from its original path. The deflection of the beam is directly releated to the frequency of rotation of the mirror and inversely related to the speed of light.

Determination of the Velocity of Radio Waves

http://did.cit.jmu.edu/default.aspx?direct=image&id=31&res=ffh01073.xml

AE5.F55 Internet

The wavelengths and frequencies of radio waves are measured from the electric and magnetic fields generated from standing electromagnetic waves in an open-circuited transmission line. The distance between successive maxima in the electric and magnetic fields is one-half the wavelength of the original radiation. These maxima are measured along the transmission line with a vertical antenna on a receiver for the electric field and with a loop antenna for the magnetic field. Students record the distances between the maxima in the receiver signal. The frequency is timed by feeding the radio wave signal from the oscillator to a frequency meter which uses a piezoelectric crystal as the timer. Students can calculate the velocity of the radio waves (the product of the wavelength and the frequency) and compare this with the velocity of light measured in Program 1, Determination of the Velocity of Light.

Determination of the Newtonian Constant of Gravitation, The

http://did.cit.jmu.edu/default.aspx?direct=image&id=31&res=ffh01074.xml

AE5.F55 Internet

The Newtonian constant of gravitation is determined by measuring the gravitational force of attraction between massive spheres of lead and mercury. A torsion balance is used to measure the deflection angle which balances the torsional couple of the balance with the gravitational couple exerted by the massive spheres.

Electron Diffraction

http://did.cit.jmu.edu/default.aspx?direct=image&id=31&res=ffh01077.xml

AE5.F55 Internet

The wave behavior of electrons is studied by measuring the diffraction ring diameters produced when accelerated electrons pass through a graphite lattice. Students record the ring diameters for different electron accelerating voltages. The wavelength of the electrons is directly related to the ring diameters. Students can also verify de Broglie's relation, which states that the electron's wavelength is Planck's constant divided by the electron's momentum since the momentum is proportional to the square root of the accelerating voltage.

Determination of a Radioactive Half-Life, The

http://did.cit.jmu.edu/default.aspx?direct=image&id=31&res=ffh01083.xml

AE5.F55 Internet

In this program students measure the radioactive half-life of a metastable indium isotope produced by the neutron irradiation of an indium foil. After the sample has been irradiated, the number of ss-rays emitted can be measured with a Geiger counter. Students record the number of clicks of the Geiger counter for one-minute periods at half-hour intervals. By plotting the logarithm of the number of counts as a function of real time, the half-life can be read directly.

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