DISTANCES TO NEARBY STARS
AND THEIR MOTIONS:
An Introductory Astronomy Lab


This lab takes you to the next step in the cosmic distance ladder: figuring out the distances to stars other than the Sun. Astronomers derive distances to the nearest stars by a form of triangulation called stellar parallax, a most simple and direct method that relies on no assumptions other than the geometry of the Earth's orbit around the sun.


The steps to follow:

References, credits, etc. will be available soon.


Written by Joachim Stadel and Luis Mendoza
1998, Astronomy Department, University of Washington

This page is maintained by Luis Mendoza .
Suggestions, comments, and questions should be sent to: mendoza@astro.washington.edu
Last update: Feb.13,1998

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