Explore a comprehensive video series on light and electromagnetic radiation in astronomy. Delve into various types of radiation, wave properties, and their production. Understand the electromagnetic spectrum, including visible light and potentially dangerous frequencies. Learn about atmospheric protection, Wien's Law, and Stefan-Boltzmann's Law. Investigate emission spectra of celestial objects, the Doppler effect, and its applications in astronomy. Discover how observing electromagnetic radiation provides crucial information about the universe and its contents.
Overview
Syllabus
Astronomy - Ch. 5: Light & E&M Radiation (1 of 30) Types of Radiation
Astronomy - Ch. 5: Light & E&M Radiation (2 of 30) Differences in Radiation
Astronomy - Ch. 5: Light & E&M Radiation (3 of 30) Important Basics Of Waves
Astronomy - Ch. 5: Light & E&M Radiation (4 of 30) What Produces E&M Waves?
Astronomy - Ch. 5: Light & E&M Radiation (5 of 30) How Are E&M Waves Produced?
Astronomy - Ch. 5: Light & E&M Radiation (6 of 30) Difference of E&M Frequence
Astronomy - Ch. 5: Light & E&M Radiation (7 of 30) What Are Frequencies of Light?
Astronomy - Ch. 5: Light & E&M Radiation (8 of 30) E&M Radiation...Safe or Dangerous?
Astronomy - Ch. 5: Light & E&M Radiation (9 of 30) How Does the Atmosphere Protect Us?
Astronomy - Ch. 5: Light & E&M Radiation (10 of 30) Differences: Transparent vs Opaque Atmosphere
Astronomy - Ch. 5: Light & E&M Radiation (11 of 30) Relationship: Radiation, Wavelength, and Opaque
Astronomy - Ch. 5: Light & E&M Radiation (12 of 30) What is Light made Of?
Astronomy - Ch. 5: Light & E&M Radiation (13 of 30) Different Energies of E&M Radiations
Astronomy - Ch. 5: Light & E&M Radiation (14 of 30) Why is UV Radiation Dangerous?
Astronomy - Ch. 5: Light & E&M Radiation (15 of 30) Wien's Law (Temperature vs Radiation)
Astronomy - Ch. 5: Light & E&M Radiation (16 of 30) Radiation Curves of Stars and Humans
Astronomy - Ch. 5: Light & E&M Radiation (17 of 30) Stefan-Botzmann Velocity Distribution
Astronomy - Ch. 5: Light & E&M Radiation (18 of 30) Stefan-Boltzmann's Law
Astronomy - Ch. 5: Light & E&M Radiation (19 of 30) Why Do Hot Objects Glow?
Astronomy - Ch. 5: Light & E&M Radiation (20 of 30) Why Light Sources have Different Spectra?
Astronomy - Ch. 5: Light & E&M Radiation (21 of 30) Emission Spectrum of Nebula
Astronomy - Ch. 5: Light & E&M Radiation (22 of 30) Emission Spectrum of Helium
Astronomy - Ch. 5: Light & E&M Radiation (23 of 30) Emission Spectrum and Amount of Elements
Astronomy - Ch. 5: Light & E&M Radiation (24 of 30) Emission Spectrum of Celestial Object
Astronomy - Ch. 5: Light & E&M Radiation (25 of 30) Doppler Shift and Celestial Movement
Astronomy - Ch. 5: Light & E&M Radiation (26 of 30) Doppler Shift and Celestial Radial Movement
Astronomy - Ch. 5: Light & E&M Radiation (27 of 30) Red Shift and Blue Shift Explained
Astronomy - Ch. 5: Light & E&M Radiation (28 of 30) Finding the Velocities of Celestial Objects
Astronomy - Ch. 5: Light & E&M Radiation (29 of 30) Doppler Shift and Rotation of Celestial Objects
Astronomy - Ch. 5: Light & E&M Radiation (30 of 30) What Can Observing E&M Radiation Tell Us?
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Taught by
Michel van Biezen
