The Mechanical Universe

The Mechanical Universe  - TV series (1985)

Original title

The Mechanical Universe

Released

1/1/1985

Genre

Documentary

Status

Ended

Number of seasons

1

Number of episodes

52

Description

The Mechanical Universe... And Beyond, is a 52-part telecourse filmed at the California Institute of Technology, and produced by Caltech and INTELECOM Intelligent Telecommunications. The series introduces university level physics, covering topics from Copernicus to quantum mechanics. Produced starting in 1985, the videos make heavy use of historical dramatizations and visual aids to explain physics concepts. The latter were state of the art at the time, incorporating almost 8 hours of computer animation created by computer graphics pioneer Jim Blinn. Each episode opens and closes with a "phantom" lecture by Caltech professor David Goodstein. After more than a quarter century, the series is still often used as a supplemental teaching aid, for its clear explanation of fundamental concepts such as special relativity. The Mechanical Universe lectures are actual freshman physics lectures from Physics 1a and 1b courses at the California Institute of Technology. The room seen in the videos is the Bridge lecture hall. The series can be purchased, or viewed by streaming from the Annenberg website, or can be viewed on other video streaming sites such as YouTube and Google Video.

Сезони

Season 1

Season 1

52 серій

01/01/1985

View episodes
Introduction

1. Introduction

01/01/1985

This preview introduces revolutionary ideas and heroes from Copernicus to Newton, and links the physics of the heavens and the earth.

The Law of Falling Bodies

01/01/1970

Galileo's imaginative experiments proved that all bodies fall with the same constant acceleration.

Derivatives

3. Derivatives

01/01/1970

The function of mathematics in physical science and the derivative as a practical tool.

Inertia

4. Inertia

01/01/1970

Galileo risks his favored status to answer the questions of the universe with his law of inertia.

Vectors

5. Vectors

01/01/1970

Physics must explain not only why and how much, but also where and which way.

Newton's Laws

6. Newton's Laws

01/01/1970

Newton lays down the laws of force, mass, and acceleration.

Integration

7. Integration

01/01/1970

Newton and Leibniz arrive at the conclusion that differentiation and integration are inverse processes.

The Apple and the Moon

01/01/1970

The first real steps toward space travel are made as Newton discovers that gravity describes the force between any two particles in the universe.

Moving in Circles

9. Moving in Circles

01/01/1970

A look at the Platonic theory of uniform circular motion.

Fundamental Forces

10. Fundamental Forces

01/01/1970

All physical phenomena of nature are explained by four forces: two nuclear forces, gravity, and electricity.

Gravity, Electricity, Magnetism

01/01/1970

Shedding light on the mathematical form of the gravitational, electric, and magnetic forces.

The Millikan Experiment

01/01/1970

A dramatic recreation of Millikan's classic oil-drop experiment to determine the charge of a single electron.

Conservation of Energy

01/01/1970

According to one of the major laws of physics, energy is neither created nor destroyed.

Potential Energy

14. Potential Energy

01/01/1970

Potential energy provides a powerful model for understanding why the world has worked the same way since the beginning of time.

Conservation of Momentum

01/01/1970

What keeps the universe ticking away until the end of time?

Harmonic Motion

16. Harmonic Motion

01/01/1970

The music and mathematics of periodic motion.

Resonance

17. Resonance

01/01/1970

Why a swaying bridge collapses with a high wind, and why a wine glass shatters with a higher octave.

Waves

18. Waves

01/01/1970

With an analysis of simple harmonic motion and a stroke of genius, Newton extended mechanics to the propagation of sound.

Angular Momentum

19. Angular Momentum

01/01/1970

An old momentum with a new twist.

Torques and Gyroscopes

01/01/1970

From spinning tops to the precession of the equinoxes.

Kepler's Three Laws

01/01/1970

The discovery of elliptical orbits helps describe the motion of heavenly bodies with unprecedented accuracy.

The Kepler Problem

22. The Kepler Problem

01/01/1970

The deduction of Kepler's laws from Newton's universal law of gravitation is one of the crowning achievements of Western thought.

Energy and Eccentricity

01/01/1970

The precise orbit of a heavenly body — a planet, asteroid, or comet — is fixed by the laws of conservation of energy and angular momentum.

Navigating in Space

01/01/1970

Voyages to other planets use the same laws that guide planets around the solar system.

Kepler to Einstein

25. Kepler to Einstein

01/01/1970

From Kepler's laws and the theory of tides, to Einstein's general theory of relativity, into black holes, and beyond.

Harmony of the Spheres

01/01/1970

A last lingering look back at mechanics to see new connections between old discoveries.

Beyond the Mechanical Universe

01/01/1970

The world of electricity and magnetism, and 20th-century discoveries of relativity and quantum mechanics.

Static Electricity

28. Static Electricity

01/01/1970

Eighteenth-century electricians knew how to spark the interest of an audience with the principles of static electricity.

The Electric Field

29. The Electric Field

01/01/1970

Faraday's vision of lines of constant force in space laid the foundation for the modern force field theory.

Potential and Capacitance

01/01/1970

Franklin proposes a successful theory of the Leyden jar and invents the parallel plate capacitor.

Voltage, Energy, and Force

01/01/1970

When is electricity dangerous or benign, spectacular or useful?

The Electric Battery

01/01/1970

Volta invents the electric battery using the internal properties of different metals.

Electric Circuits

33. Electric Circuits

01/01/1970

The work of Wheatstone, Ohm, and Kirchhoff leads to the design and analysis of how current flows.

Magnetism

34. Magnetism

01/01/1970

Gilbert discovered that the earth behaves like a giant magnet. Modern scientists have learned even more.

The Magnetic Field

35. The Magnetic Field

01/01/1970

The law of Biot and Sarvart, the force between electric currents, and Ampère's law.

Vector Fields and Hydrodynamics

01/01/1970

Force fields have definite properties of their own suitable for scientific study.

Electromagnetic Induction

01/01/1970

The discovery of electromagnetic induction in 1831 creates an important technological breakthrough in the generation of electric power.

Alternating Current

01/01/1970

Electromagnetic induction makes it easy to generate alternating current while transformers make it practical to distribute it over long distances.

Maxwell's Equations

01/01/1970

Maxwell discovers that displacement current produces electromagnetic waves or light.

Optics

40. Optics

01/01/1970

Many properties of light are properties of waves, including reflection, refraction, and diffraction.

The Michelson-Morley Experiment

01/01/1970

In 1887, an exquisitely designed measurement of the earth's motion through the ether results in the most brilliant failure in scientific history.

The Lorentz Transformation

01/01/1970

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.

Velocity and Time

43. Velocity and Time

01/01/1970

Einstein is motivated to perfect the central ideas of physics, resulting in a new understanding of the meaning of space and time.

Mass, Momentum, Energy

01/01/1970

The new meaning of space and time make it necessary to formulate a new mechanics.

Temperature and Gas Laws

01/01/1970

Hot discoveries about the behavior of gases make the connection between temperature and heat.

Engine of Nature

46. Engine of Nature

01/01/1970

The Carnot engine, part one, beginning with simple steam engines.

Entropy

47. Entropy

01/01/1970

The Carnot engine, part two, with profound implications for the behavior of matter and the flow of time through the universe.

Low Temperatures

48. Low Temperatures

01/01/1970

With the quest for low temperatures came the discovery that all elements can exist in each of the basic states of matter.

The Atom

49. The Atom

01/01/1970

A history of the atom, from the ancient Greeks to the early 20th century, and a new challenge for the world of physics.

Particles and Waves

01/01/1970

Evidence that light can sometimes act like a particle leads to quantum mechanics, the new physics.

From Atoms to Quarks

01/01/1970

Electron waves attracted to the nucleus of an atom help account for the periodic table of the elements and ultimately lead to the search for quarks.

The Quantum Mechanical Universe

01/01/1970

A last look at where we've been and a peek into the future.

Images

/pCF6G2F3dh0qKDg4476DWVLI7ML.jpg

Recommendations

The Simpsons

The Simpsons

12/17/1989

Breaking Bad

Breaking Bad

1/20/2008

Twin Peaks

Twin Peaks

4/8/1990

Lost

Lost

9/22/2004

Dragon Ball Z

Dragon Ball Z

4/26/1989

Black Mirror

Black Mirror

12/4/2011

WandaVision

WandaVision

1/15/2021

Chernobyl

Chernobyl

5/6/2019

Bridgerton

Bridgerton

12/25/2020

Moon Knight

Moon Knight

3/30/2022

Squid Game

Squid Game

9/17/2021

Arcane

Arcane

11/6/2021

Asset 4

This website uses TMDB and the TMDB APIs but is not endorsed, certified, or otherwise approved by TMDB.