ASTR 3 Lecture Notes - Lecture 4: 30 Foot Fall, Photon, Planetary Science

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28 Aug 2016
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Each type of atom has a unique set of energy levels. Each transition corresponds to a unique photon energy, frequency, and wavelength. Each individual element is unique in the amount of energy is absorbs (but the same types of elements absorb the same amount all hydrogen atoms, all helium atoms, etc) Molecules have additional energy levels because they can vibrate and rotate. How does light tell us what things are made of: each atom has a unique ngerprint, we can determine which atoms something is made of by looking for their. How does light tell us the temperature of planets and stars: nearly all large or dense objects emit a continuous spectrum that depends on temperature, the spectrum of that thermal radiation tells us the object"s temperature. How does light tell us the speed of a distant object: the doppler affect tells us how fast an object is moving towards or away from us.

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