Light: Electromagnetic spectrum & Doppler Shift

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Presentation transcript:

Light: Electromagnetic spectrum & Doppler Shift

The Electromagnetic Spectrum

Cosmic Background Radiation (CBR) The hypothesis that the universe has always been expanding (since the “Big Bang”) predicted (1948) that radiation produced from the first moment of expansion would permeate the universe. In 1965 this radiation was discovered In 2003 astronomers studying the CBR determined the universe is 13.7 billion years old

Cosmic Speed Limit Speed of light = 300,000 km/s Light-year = the distance light travels in one year = 9,500,000,000,000 km The 2nd nearest star is 4.3 light years away

Spectrum: light separated into component wavelengths Droplets of water, diffraction grating, and spectroscopes all act like a PRISM to separate different wavelengths (colors) of light

Incandescence: glowing from heat Blue = hottest Red=coolest

Types of spectra Sunlight, light bulbs Sunlight that has traveled through our atmosphere Hot gas

Doppler Effect Pitch: higher Light: bluer Pitch: Lower Light: redder

Doppler shifts from stars