Relay-Version: version B 2.10 5/3/83; site utzoo.UUCP Posting-Version: version B 2.10.2 9/5/84; site mordor.UUCP Path: utzoo!linus!philabs!cmcl2!seismo!lll-crg!mordor!@S1-A.ARPA,@MIT-MC.ARPA:koolish@bbncd2 From: @S1-A.ARPA,@MIT-MC.ARPA:koolish@bbncd2 Newsgroups: net.space Subject: obliquity of the ecliptic Message-ID: <2890@mordor.UUCP> Date: Wed, 31-Jul-85 16:22:24 EDT Article-I.D.: mordor.2890 Posted: Wed Jul 31 16:22:24 1985 Date-Received: Fri, 2-Aug-85 06:56:48 EDT Sender: daemon@mordor.UUCP Organization: S-1 Project, LLNL Lines: 33 From: Dick Koolish To get back to the original question that brought on all the discussion about the Gregorian calendar: The earths axis of rotation is subject to precession and change of tilt. Both these effects would change the way that ancient structures line up with astronomical objects. The difference is that precession changes the positions of stars while tilt changes the position of the sun. Precession causes the pole to describe a circle in the sky instead of remaining fixed at one place. This causes the positions of stars and constellations to change. Polaris is the pole star now because the axis is pointing near Polaris. 13,000 years ago, it was on the other side of the precessional circle. In the 2,000 years or so since the constellations were named, precession has moved around the zodiac by a full constellation so that none of the astrological signs correspond to where the sun really is in the sky. The tilt or obliquity of the ecliptic also changes. This is a long period change of 41,000 years that takes the tilt from 24.5 degrees to 22.1 degrees at about .47 seconds per year. This change of tilt affects solar phenomena like sunrise, sunset, etc. The formula for the tilt is: 23 degrees 26 minutes 21.448 seconds - 46.8150*T seconds - .00059*T*T seconds + .001813*T*T*T seconds where T is the number of Julian centuries from 2000