Relay-Version: version B 2.10 5/3/83; site utzoo.UUCP Path: utzoo!mnetor!seismo!lll-crg!rutgers!clyde!burl!codas!mtune!mtuxo!houxm!ho95e!ran From: ran@ho95e.UUCP (RANeinast) Newsgroups: sci.physics Subject: Re: Accelerating elevator Message-ID: <1132@ho95e.UUCP> Date: Fri, 14-Nov-86 14:44:27 EST Article-I.D.: ho95e.1132 Posted: Fri Nov 14 14:44:27 1986 Date-Received: Sun, 16-Nov-86 00:11:28 EST References: <1388@trwrb.UUCP> <546@mcgill-vision.UUCP> <1167@cit-vax.Caltech.Edu> Organization: AT&T Bell Labs, Holmdel NJ Lines: 26 > Hey, here's a fairly interesting question! What happens to the background > black-body radiation when you start moving faster? Obviously, it gets > doppler shifted. What does the distribution of radiation with wavelength > look like? Is it still a black-body curve? > All sorts of interesting questions with this one! > -Bob Myers A Doppler shifted blackbody curve (actually, it can be shifted by any "geometric" means, such as gravitational redshift) is another blackbody curve, but with a new temperature shifted exactly as the frequencies are shifted. This means that if you look ahead of you, you will see a blackbody curve for a higher temperature, and if you look behind, you will see a blackbody curve for a lower temperature. This directional anisotropy (although quite small) has been detected in the background 3 degree radiation, and is generally interpreted as the cumulative (from motion about the sun, center of galaxy, galactic group) speed of the earth relative to the original big bang. -- ". . . and shun the frumious Bandersnatch." Robert Neinast (ihnp4!ho95c!ran) AT&T-Bell Labs