CHEM 4005 Lecture Notes - Lecture 3: Fraunhofer Lines, Electromagnetic Spectrum, Radiant Energy

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8 Jun 2017
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Any form of radiant energy in the electromagnetic spectrum. Gamma, x- rays, ultraviolet, visible, infrared, microwave, radio. Distance from crest to crest or trough to trough on a wave. Number of crests of a wave that pass a stationary point reference per second. Dark lines in the otherwise continuous solar spectrum. Pattern of bright lines produced when atoms are vaporized in high temperature flames. Pattern of dark lines produced when an external source of radiation passes through free, gaseous atoms. The smallest discrete quantity of a particular form of energy. Having values restricted to whole- number multiples of a specific base value. Most stable, lowest energy state of a particle. Principle that one cannot simultaneously know the exact position and the exact momentum of an electron. One of four related numbers that specify the energy, shape and orientation of orbitals in an atom. Main energy level, shell or distance from center.

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