Black Holes, Tides, and Curved Spacetime: Understanding Gravity

Black Holes, Tides, and Curved Spacetime: Understanding Gravity « Series from 2013

Series from 2013

Broadcast info
Genres: Special Interest

Gravity rules the universe. Without it, everything would dissolve into a gas of randomly interacting atoms. Yet gravity is one of the least understood forces in nature.

Black Holes, Tides, and Curved Spacetime introduces you to key ideas in gravity research over the past 400 years. It's an awe-inspiring journey led by a prominent theoretical physicist.

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The Strangest Force

Begin your exploration of gravity with Isaac Newton and the famous story of the apple. Why was it such a breakthrough to connect a falling apple with the faraway moon? Review the essential characteristics of gravity and learn why small asteroids and large planets have such different shapes.

Free Fall and Inertia

Review three great discoveries by the "grandfather" of gravity research, Galileo Galilei. His most famous experiment may never have happened, but his principle of inertia, law of free fall, and principle of relativity are the basis for everything that comes later in the science of gravity - including key breakthroughs by Einstein.

Revolution in the Heavens

Drawing on ideas and observations of Nicolaus Copernicus and Tycho Brahe, Johannes Kepler achieved a great insight about gravity by discovering three laws of planetary motion, relating to the mathematics of orbits. The cause of planetary motion, he determined, must lie in the sun.

Universal Gravitation

See how Newton was able to finish Kepler's revolution by formulating the law of universal gravitation, which says that every object exerts an attractive force on every other object. Also explore Newton's related discovery of the three laws of motion, which underlie the science of mechanics.

The Art of Experiment

Learn how distances in the solar system were first determined. Then chart Henry Cavendish's historic experiment that found the value of Newton's gravitational constant. Cavendish's work allows almost everything in the universe to be weighed. Then see a confirmation of the equivalence principle, which says that gravitational and inertial mass are identical.

Escape Velocity, Energy, and Rotation

Begin to dig deeper into Newton's laws than Newton himself was able to go. Here, apply the key concepts of energy and angular momentum to study how gravity affects motion. As an example, use simple algebra to calculate the escape velocity from Earth.

Stars in Their Courses--Orbital Mechanics

What Are Tides? Earth and Beyond

Nudge--Perturbations of Orbits

Resonance--Surprises in the Intricate Dance

The Million-Body Problem

The Billion-Year Battle

From Forces to Fields

The Falling Laboratory

Spacetime in Zero Gravity

Spacetime Tells Matter How to Move

Matter Tells Spacetime How to Curve

Light in Curved Spacetime

Gravitomagnetism and Gravitational Waves

Gravity's Horizon--Anatomy of a Black Hole

Which Universe Is Ours?

Cosmic Antigravity--Inflation and Dark Energy

The Force of Creation

The Next Revolution