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In order to understand how we study the universe, we need to talk a little bit about light. Light is a form of energy. Its wavelength tells us its energy and color. Spectroscopy allows us to analyze those colors and determine an object’s temperature, density, spin, motion, and chemical composition.
Check out the Crash Course Astronomy solar system poster here: store.dftba.com/products/crash...
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Chapters:
Introduction 00:00
Light is a Wave 0:31
Electromagnetic Spectrum 1:32
How is Light Made? 3:19
Atomic Structure 4:47
Spectroscopy 7:14
Redshift vs Blueshift 8:26
Review 9:50
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PHOTOS/VIDEOS
Wavelengths imagine.gsfc.nasa.gov/educator... [credit: Imagine the Universe! / NASA]
Observatories across spectrum imagine.gsfc.nasa.gov/Images/s... [credit: Imagine the Universe! / NASA]
Red hot spiral hotplate freefoodphotos.com/imagelibrar... [credit: freefoodphotos.com]
The Crab Nebula en.wikipedia.org/wiki/Nebula#/... [credit: NASA, ESA, J. Hester and A. Loll (Arizona State University)]
Building the Space Telescope Imaging Spectograph imgsrc.hubblesite.org/hu/galle... [credit: NASA]
VST images the Lagoon Nebula en.wikipedia.org/wiki/Lagoon_N... [credit: ESO/VPHAS+ team]
Jupiter www.nasa.gov/images/content/41... [credit: NASA/Johns Hopkins University Applied Physics Laboratory/Southwest Research Institute]
Venus en.wikipedia.org/wiki/Atmosphe... [credit: NASA - NSSDC Photo Gallery Venus]
Ring Around SN 1987a, image 1 www.spacetelescope.org/images/... [credit: Jason Pun (NOAO) and SINS Collaboration]
Ring Around SN 1987a, image 2 www.spacetelescope.org/images/... [credit: George Sonneborn (GSFC) and NASA/ESA]