Relay-Version: version B 2.10 5/3/83; site utzoo.UUCP Posting-Version: version B 2.10.1 6/24/83; site kpnoa.UUCP Path: utzoo!watmath!clyde!burl!ulysses!mhuxl!ihnp4!zehntel!hplabs!hao!noao!kpnoa!parks From: parks@kpnoa.UUCP Newsgroups: net.astro.expert Subject: Stability of the 'Nemesis' system Message-ID: <339@kpnoa.UUCP> Date: Thu, 24-May-84 12:57:11 EDT Article-I.D.: kpnoa.339 Posted: Thu May 24 12:57:11 1984 Date-Received: Thu, 31-May-84 20:00:51 EDT Organization: Natl. Optical Astronomy Observatories Tucson AZ USA Lines: 21 I have in my hands a preprint of a paper by Piet Hut (from Princeton) concerning the possibility of a companion star which orbits ours at about a light year out. I'm not sure, but I believe this is being submitted to Letters to the Astrophysical Journal, so it may appear in print in about six months. The current title for the article is "How stable is an astronomical clock which can trigger mass extinctions on earth?". It seems he will also be publishing a more detailed analysis of his calculations (although I don't know where). I don't want to reveal too much of his paper (get your own pre-print), but he has done extensive computer simulations on a VAX 11/780, including: over 10^7 stellar encounters, the galactic tidal field, and various orbit orientations to the galactic plane. After studying these effects, he concludes that such a system IS possible, although it should come apart in time. A related factor to its instability is that the period is not precisely regular, but may vary as much as 20%. Jay Parks (decvax!hao!ihnp4!seismo)!noao!parks :uucp