Path: utzoo!utgpu!news-server.csri.toronto.edu!cs.utexas.edu!usc!zaphod.mps.ohio-state.edu!mips!spool.mu.edu!snorkelwacker.mit.edu!stanford.edu!rutgers!soleil!mlb.semi.harris.com!solman.mlb.semi.harris.com!bie From: bie@solman.mlb.semi.harris.com (Ben Eaton) Newsgroups: sci.electronics Subject: RE: How to tell distance of Stars Message-ID: <1991May16.191838.2265@mlb.semi.harris.com> Date: 16 May 91 19:18:38 GMT Sender: news@mlb.semi.harris.com Organization: Harris Semiconductor, Melbourne FL Lines: 30 Nntp-Posting-Host: solman.mlb.semi.harris.com If memory serves me correctly there are three common methods used to determine the distance to individual stars. A) PARALLAX In this method you measure the apparent shift in position of a star in relation to other background stars as the earth moves around the sun. This method is only good out to about one to two hundred light years. B) COLOR VERSUS LUMINOSITY In this method you measure the apparent luminosity of a star and compare it to a star of the same color with a known distance and use the inverse square law to calculate the distance. This works within our own galaxy but outside of that I don't know. C) PERIOD VERSUS LUMINOSITY This method only works for variable stars and is just like the color versus luminosity method only you compare stars of like periods. This works for as far out as you can see the individual star. I hope this will be of some help if you want more get in contact with a community collage that has an astronomy department. Ben