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9/19
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How to measure the distance and energy of stars using blackbody radiation, spectral line emissions, and light wavelengths, explaining the greenhouse effect
Class notes
9/19
Last document update:
ago
How to measure the distance and energy of stars using blackbody radiation, spectral line emissions, and light wavelengths, explaining the greenhouse effect
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R115 for your summary multiplied by 100 fellow students... Do the math: that's a lot of money! Don't be a thief of your own wallet and start uploading yours now. Discover all about earning on Stuvia