Relay-Version: version B 2.10 5/3/83; site utzoo.UUCP Path: utzoo!mnetor!seismo!lll-crg!nike!sri-spam!sri-unix!hplabs!tektronix!uw-beaver!ubc-vision!ubc-cs!majka From: majka@ubc-cs.UUCP Newsgroups: sci.astro Subject: Re: problem: a view from a planet Message-ID: <442@ubc-cs.UUCP> Date: Wed, 15-Oct-86 15:07:47 EDT Article-I.D.: ubc-cs.442 Posted: Wed Oct 15 15:07:47 1986 Date-Received: Fri, 17-Oct-86 04:00:45 EDT References: <7751@tekecs.TEK.COM> Reply-To: majka@ubc-cs.UUCP (Marc Majka) Organization: UBC Department of Computer Science, Vancouver, B.C., Canada Lines: 11 A planet with a rotational axis in the plane of the solar ecliptic is possible. To get one side always facing the sun would require the sun to be always along the rotational axis, with a precession matching the length of the planet's year. Thus it would appear to always be either due north or due south of any observer. It would not revolve in circles with size growing larger away from the poles. Rather is would remain in a stationary position, as Polaris appears from Earth. However, it would appear to spin in place. --- Marc Majka