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Classical Mechanics - Lecture 23

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Lecture 23 - Doppler Effect

Doppler Effect, Binary Stars, Neutron Stars and Black Holes. Doppler shift is introduced with sound waves, then extended to electromagnetic waves (radiation). The Doppler shift of stellar spectral lines and/or pulsar frequencies provides a measure of the line-of-sight (so-called radial) velocity of the source relative to the observer. Combined with Newton's law of universal gravitation, this can lead to the orbital parameters and the mass of both stars in a binary star system.

Prof. Walter Lewin
8.01 Physics I: Classical Mechanics, Fall 1999
(Massachusetts Institute of Technology: MIT OpenCourseWare)
http://ocw.mit.edu
Date accessed: 2008-12-12
License: Creative Commons BY-NC-SA

Lecture Material

Supplementary lecture material is listed below.

1. Effects of Inclination of Binary Systems



 

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