Relay-Version: version B 2.10 5/3/83; site utzoo.UUCP Posting-Version: version B 2.10.2 9/18/84; site voder.UUCP Path: utzoo!watmath!clyde!burl!ulysses!mhuxj!ihnp4!zehntel!dual!amd!fortune!hpda!hplabs!nsc!voder!gino From: gino@voder.UUCP (Gino Bloch) Newsgroups: net.astro Subject: Re: Measurement of Light Years and Distance Message-ID: <479@voder.UUCP> Date: Fri, 26-Oct-84 21:09:01 EST Article-I.D.: voder.479 Posted: Fri Oct 26 21:09:01 1984 Date-Received: Sun, 28-Oct-84 06:48:00 EST References: <872@ihuxp.UUCP> Organization: National Semiconductor, Santa Clara Lines: 23 > Can anyone tell me how the distance in light years is measured? > How do we know how far something is? Does the spectrum shift > of light have something to do with it? > F. C. McAtee Not a trivial question. In short: distances are measured by a long chain of difficult measurements, deductions, and extrapolations, where the term `noise-to-signal ratio' would be more appropriate than the usual term. At greater length: the first step is parallax, the apparent shift in position of objects viewed from opposite sides of the earth's ORBIT. This is good to a few hundred light years with decreasing accuracy. After that, knowledge of such things as brightness as a function of spectral class and other characteristics is used. The latter leads to distance to nearer galaxies, such as Andromeda (M31). Properties of galaxies as a whole lead to estimates for farther galaxies and clusters. Finally, the red-shift observed in this regime leads to extrapolation of distances to the farthest galaxies. The above just scratches the surface to give a flavor of what goes on. Read some good books on astronomy (I have no recommendations at my finger- tips, sorry). That will be fun, I think (but then I love astronomy). -- Gene E. Bloch (...!nsc!voder!gino)