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back to Tour the Universe Galaxies are the building blocks of the universe. Clusters of galaxies, and clusters of clusters of galaxies, called superclusters, make up the structures in the geography of the universe. In this section, we'll explore these structures and take a look at our address on these scales. Galaxies are titanic swarms of tens of millions to trillions of stars. Between the stars, there can be vast interstellar clouds of gas and dust. Spiral galaxies have a thin, pancake-shaped disk, with a spherical bulge at the center. Within the disk, the brightest stars trace out the characteristic spiral pattern. Elliptical galaxies are shaped roughly like watermelons, some round and some elongated. Large galaxies are approximately 100 thousand light-years across (a light-year is the distance light travels in one year: about six trillion miles). In rather plain fashion, the smallest galaxies are called dwarfs while the largest are called giants. Our Milky Way Galaxy is one of three large galaxies in the Local Group of Galaxies. The other large galaxies are the Andromeda Galaxy, and Messier 33 (the 33rd entry in Charles Messier's catalog of fuzzy things in the sky). Also in the Local Group are a couple dozen dwarf galaxies. Several of these dwarf galaxies are satellite galaxies, orbiting around the large galaxies. The Milky Way has two prominent satellite galaxies, called the Large and Small Magellanic Clouds. (The Magellanic Clouds are visible on Earth only from the southern hemisphere; their existence was recorded by the voyage of Magellan). The Local Group is a small clustering of galaxies, a few million light-years across. Larger clusters of galaxies can contain hundreds of galaxies. Galaxies within a cluster are generally considered to be bound together by their mutual gravitational pulls. They each orbit around their common center of mass. Because the density of galaxies is high within clusters, galaxy collisions occur. One such collision can be seen in the lower right of the image of the Virgo cluster below.
The enormous gravity of the Virgo Cluster makes it the center of a larger structure, called the Local Supercluster. This collection of nearly 100 clusters, and thousands of galaxies, stretches across a hundred million light-years. The Local Group is just a tiny member of the Virgo Supercluster, located on the outskirts. Just as we have found that Earth is not the center of the solar system, and the Sun is just another star in the Milky Way, so too have we found that our galaxy holds no special place in the universe.
The 3-D model below will show you the structure of about 1,800 nearby galaxies. Our data sets have good 3-D positions for about 35,000 galaxies. Large galaxy surveys are attempting to measure millions of galaxies and map their distribution in space. We are only beginning to learn and explore the geography of the universe. Let's get going. Background Galaxies, Clusters, and Superclusters How is the Universe structured? Find out here. The Local Universe in 3-D: A VRML Tour Preparing Yourself and Your Computer for VRML Where to get the VRML plugin, system requirements, and how to navigate through a 3-D VRML world. The Local Universe in 3-D (VRML; 151Kbytes) Jump right into the tour if your computer already has a VRML plugin installed. Non-VRML Version Zoom-Out Map of the Local Universe Travel millions of light years away from Earth in this simple graphic and text version of the tour. Photos: (1-4) AURA/NOAO/NSF; (5) NASA/STScI. History of the Universe | Birth of a Supernova | Tour the Universe Moving Targets | How Big is the Universe? | Spin a Spiral Galaxy Resources | Transcript | Site Map | Runaway Universe Home Editor's Picks | Previous Sites | Join Us/E-mail | TV/Web Schedule About NOVA | Teachers | Site Map | Shop | Jobs | Search | To print PBS Online | NOVA Online | WGBH © | Updated November 2000 |
