Relay-Version: version B 2.10 5/3/83; site utzoo.UUCP Posting-Version: version B 2.10.2 9/18/84; site ames.UUCP Path: utzoo!watmath!clyde!burl!ulysses!allegra!bellcore!decvax!genrad!panda!talcott!harvard!seismo!hao!ames!eugene From: eugene@ames.UUCP (Eugene Miya) Newsgroups: net.astro Subject: Re: StarDate: April 24 Nine Months to Uranus Message-ID: <971@ames.UUCP> Date: Mon, 6-May-85 17:57:46 EDT Article-I.D.: ames.971 Posted: Mon May 6 17:57:46 1985 Date-Received: Thu, 9-May-85 02:28:06 EDT References: <55@utastro.UUCP> <603@abnji.UUCP> Organization: NASA-Ames Research Center, Mtn. View, CA Lines: 27 > When I read this, it seemed a bit misleading. As Uranus moves around its > orbit, one hemisphere gradually lightens and one gradually darkens. In > fact, most of the time, most of the planet will get sunlight in a given day. > Most? Maybe close to 50%? Half a sphere if we 'round' the oblate structure of the planet. > > In the case of Uranus, the Arctic circle is much farther south, so > this effect is more pronounced. > -- > James C Armstrong, Jnr. ihnp4!abnji!nyssa I think the difficulty came in describing the 72 degree axis tilt of Uranus [if my memory does not fail me]. One of the last things I did before leaving JPL was begin the preliminary planning for the simulation of Uranus encounter. There are several unknowns regarding the length of the Uranian day, I think we found four different lengths of a day. Seasons are not well understood. It would help immensly if it were possible to see planetary features thru ground-based telescopes (or space-based). Oh! to have digitized pictures of StarDate transmissions rather than the text. Debbie should illustrate using computer generated animation. Will Bill Skane of Science notes on PBS do the same? --eugene miya NASA Ames Research Center {hplabs,ihnp4,dual,hao,decwrl,allegra}!ames!aurora!eugene emiya@ames-vmsb.ARPA