Relay-Version: version B 2.10 5/3/83; site utzoo.UUCP Posting-Version: version B 2.10.2 9/18/84 exptools; site ihlpa.UUCP Path: utzoo!watmath!clyde!burl!ulysses!mhuxr!mhuxb!houxm!ihnp4!ihlpa!lew From: lew@ihlpa.UUCP (Lew Mammel, Jr.) Newsgroups: net.astro Subject: Re: precession of perihelion Message-ID: <131@ihlpa.UUCP> Date: Mon, 25-Feb-85 14:55:13 EST Article-I.D.: ihlpa.131 Posted: Mon Feb 25 14:55:13 1985 Date-Received: Wed, 27-Feb-85 08:34:45 EST References: <183@npois.UUCP> Organization: AT&T Bell Laboratories Lines: 10 I believe that the time of perihelion is most simply measured by recording the time of occurrence of the equinoxes and solstices. For example, if the winter solstice occurs at perihelion there will be less time between autumnal and vernal equinoxes than vice versa. I think Aristarchus measured the eccentricity of the earth's orbit in this way. Measuring the change in the duration of the intervals would be the next step, I suppose. Lew Mammel, Jr. ihnp4!ihlpa!lew ( I'm back )