Relay-Version: version B 2.10 5/3/83; site utzoo.UUCP Posting-Version: version B 2.10.3 4.3bsd-beta 6/6/85; site utastro.UUCP Path: utzoo!watmath!clyde!burl!ulysses!bellcore!decvax!decwrl!ucbvax!im4u!ut-sally!utastro!dipper From: dipper@utastro.UUCP (Debbie Byrd) Newsgroups: net.astro Subject: StarDate: Message-ID: <561@utastro.UUCP> Date: Sat, 22-Mar-86 02:00:16 EST Article-I.D.: utastro.561 Posted: Sat Mar 22 02:00:16 1986 Date-Received: Tue, 25-Mar-86 03:47:29 EST Organization: U. Texas, Astronomy, Austin, TX Lines: 36 Invisible potholes may have formed galaxies and influenced their behavior. We'll tell you how -- after this. March 6 The Birth of the Galaxies The vast size of a galaxy is difficult to comprehend. Some, including our own Milky Way, are hundreds of thousands of light-years across. But it's even more mind-boggling to reflect on the countless billions of galaxies in our universe. Galaxies generally come in clusters. Clusters of galaxies group together on the scale of the whole universe to create a spectacular cosmic tapestry. We can observe galaxies -- but no one is sure how they came to be. Galaxy formation has always been a puzzle. But recently advances have been made toward a solution to the puzzle. In one current model, the universe started out with 90 per cent cold, dark, invisible matter and l0 per cent ordinary matter. The cold, dark matter contained locations of high density which may have acted as gravitational potholes to trap ordinary matter. Ordinary matter -- heated in the potholes -- may have evolved into galaxies. The new model suggests that the potholes tended to move towards each other and merge. Those formed early in the history of the universe were shallow -- and their galaxies merged quickly into larger structures. Later, deeper potholes formed which moved more slowly towards each other. Developing galaxies therefore had more time to cool and condense before collisions occurred. The result was not a merger but a dense clustering of galaxies. This speculation may explain why certain kinds of galaxies appear more often in dense clusters and why other kinds are more likely to be found with fewer neighbors nearby. Script by Holly Clark. (c) Copyright 1985, 1986 McDonald Observatory, University of Texas at Austin