Jason Shilling Kendall: Citizen Astronomer

William Paterson University
Amateur Astronomers Association of New York

William Paterson University

Jason Kendall is adjunct instructor of Astronomy at William Paterson University.

Jason is teaching one section of General Astronomy in the Fall of 2019:

Online Introductory Astronomy Class

CRN: 44146, PHYS 1700-81, Online lectures and laboratory activities.

Modules: Home | Books | Labs | Modules: 1 | 2 | 3 | 4 | 5 | 6 | 7 | 8 | 9 | 10 | 11 | 12 | 13 | 14 | Extra

Module 14: The Rise of Relativity

Supplements and Credits

Supplement the videos with "OpenStax Astronomy"

01: Faraday, Maxwell and the Aether

Michael Faraday and James Clerk Maxwell finalize and culminate the wave theory of light. Faraday gives us our best picture of how light “looks” and Maxwell gives us the four equations that unify electricity, magnetism and light. Also, Herchel’s discovery of infrared, and others too!

02: The Speed of Light and the Michelson Morley Experiment

What is the speed of light? What do the waves of light travel in? What do we know about how light gets here from there? The answers are even more puzzling. In this one, we learn that the waves of light can still be waves, even if they don’t actually “wave” anything. Nature starts to show us just how strange she is.

03: The Great Relativistic Conundrum

Once upon a time, there was classical physics. It had Galilean Relativity, Newtonian Mechanics and Maxwell's Laws of Electromagnetism. But, these three things, while wildly successful, did not fit together at all. Let's see why.

04: Special Relativity's Implications

Wherein we chat about the postulates of Special Relativity, and three of its main implications: desynchronization of clocks, time dilation and length contraction. Here are some good resources for special relativity.

05: Special Relativity in Detail

Wherein we detail the effects of time dilation, length contraction and clock desynchronization. We also chat about muon decay which demonstrates this effect.

06: General Relativity Raison d'être

General Relativity arises out of our need to reconcile the issues of Newtonian Gravity. It has some problems that only rethinking Gravity can solve.

07: General Relativity Curvature and Tests

General Relativity is one of the most successful theories of Physics. It helps us give a mechanism to gravity, and allows for testable predictions. We'll chat about the Correspondence Principle, The Equivalence Principle, intertial versus gravitational mass, and the nature of spacetime curvature and how it's measured. We'll chat about various tests of general relativity, and how they showed that it's the best explanation so far to the nature of space, time and gravity.

08: General Relativity: The Bending of Light's Path

General Relativity has many interesting results. In this first of two, I try to show how we can more intuitively understand what curvature of spacetime means. In this one, we look at the Equivalence Principle and show how it requires that light's path is bent according to a distant observer, but if you're falling along with the light, the path looks straight to you

09: General Relativity, The Slowing of Time by Gravity

We chat about how light is redshifted as it rises out of a gravity well, and how time runs slower in a gravity well compared to clocks far away. We also dare to ask "into where does space curve."

10: The Tides

Wherein we discuss the nature of the tides and what causes them.

William Paterson University Department of Physics American Astronomical Society Amateur Astronomers Association of New York Astronomical Society of the Pacific