Relay-Version: version B 2.10 5/3/83; site utzoo.UUCP Path: utzoo!watmath!clyde!cbosgd!gatech!ut-sally!utastro!matt From: matt@utastro.UUCP (Matt Wood) Newsgroups: net.physics Subject: Re: A Thought Experiment (Supernova) Message-ID: <337@utastro.UUCP> Date: Thu, 6-Feb-86 12:21:36 EST Article-I.D.: utastro.337 Posted: Thu Feb 6 12:21:36 1986 Date-Received: Fri, 7-Feb-86 21:31:45 EST References: <2026@teddy.UUCP> Distribution: net Organization: U. Texas, Astronomy, Austin, TX Lines: 37 Summary: blinded by the light In article <2026@teddy.UUCP>, srk@teddy.UUCP writes: > Assume there are two stars, A and B, of equal mass. They are close enough to > have significant gravitational attraction, but far enough apart that it takes > light a week or two to travel from one to the other. They are not in mutual > orbit but are approaching each other head on. This is obviously not a stable > situation! > > Star B undergoes supernova. > > At a safe distance, equidistant from both A and B, is an observer who decides > to measure these two stars immediately after the light from the supernova > passes his planet (he was watching a soap opera at the time...). He measures > the mass and acceleration of both stars. > > What will he see? > While the supernova is bright, it will shine about as brightly as the rest of the stars in the galaxy. A "safe distance" from such an event is about 10 light years, so if the stars a one light week apart, he'd probably see a single point of light. Now if we assume that we've got this great shielding on our ship and could get in close (~1 light year, this would give us good angular resolution), then roughly one year and 1 month after the explosion we'd see this shell of gas racing towards us at ~30,000 km/s. Seriously though, Ethan Vishniac gave you the theoretically-"correct" answer that I'll bet you were looking for, that ejecta already past star A will no longer affect the mechanics of the system. In fact, since after a year we'll observe the ejecta to be well past star A, we might note that A is no longer accelerating at all noticably, unless B left behind a newborn neutron star. -- Matt A. Wood Astronomy Dept, University of Texas, Austin TX 78712 {allegra,ihnp4}!{ut-sally,noao}!utastro!matt (UUCP) matt@astro.UTEXAS.EDU. (Internet)