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Table of contents

The Nature of Light

Guiding Questions

Determining the Speed of Light

Light travels through empty space at a speed of 300,000 km/s

Slide 5

Light is electromagnetic radiation and is characterized by its wavelength ()

Wavelength and Frequency

Slide 8

Slide 9

Three Temperature Scales

An opaque object emits electromagnetic radiation according to its temperature

Slide 12

Wien’s law and the Stefan-Boltzmann law are useful tools for analyzing glowing objects like stars

Wien’s Law

Slide 15

Stefan-Boltzmann Law

Slide 17

Light has properties of both waves and particles

Photons

Each chemical element produces its own unique set of spectral lines

Slide 21

Kirchhoff’s Laws

Slide 23

Slide 24

Slide 25

Slide 26

An atom consists of a small, dense nucleus surrounded by electrons

Slide 28

Slide 29

Spectral lines are produced when an electron jumps from one energy level to another within an atom

Slide 31

Slide 32

Bohr’s formula for hydrogen wavelengths

Slide 34

Balmer Lines in Star Spectrum

The wavelength of a spectral line is affected by the relative motion between the source and the observer

Doppler Shifts

Key Words

Author: Michael Cohen

E-mail: mrcohe@ship.edu

Homepage: http://physics.ship.edu/~mrc/