Relay-Version: version B 2.10 5/3/83; site utzoo.UUCP Posting-Version: version B 2.10.1 6/24/83; site utastro.UUCP Path: utzoo!linus!philabs!cmcl2!seismo!ut-sally!utastro!ethan From: ethan@utastro.UUCP (Ethan Vishniac) Newsgroups: net.astro Subject: Re: Hubble's constant Message-ID: <786@utastro.UUCP> Date: Thu, 15-Nov-84 10:37:02 EST Article-I.D.: utastro.786 Posted: Thu Nov 15 10:37:02 1984 Date-Received: Sat, 17-Nov-84 19:46:33 EST References: <646@watdcsu.UUCP> Organization: UTexas Astronomy Dept., Austin, Texas Lines: 24 [] [Herb Chong] >What's the current best value for the Hubble constant? The canonical range of 50-100 km/sec/Mpc has not been significantly narrowed in recent years. Part of the problem is that each of the extreme values has a small group of ardent partisans who continue to get their favorite value (with small error bars) each time they try a new method. One of the best efforts in recent years by an unprejudiced group of observers found that their best estimate could be varied from 65 to 90 by changing the local calibration of the Cepheid luminosity. (These are variable stars with a period - luminosity correlation.) The distances to the local Cepheids are known through a variety of indirect distance estimators. This particular uncertainty may only disappear when accurate parallax measurements become possible on these stars. There are many other sources of uncertainty. I take the arithmetic mean myself. "I can't help it if my Ethan Vishniac knee jerks" {charm,ut-sally,ut-ngp,noao}!utastro!ethan Department of Astronomy University of Texas Austin, Texas 78712