A Matter of Scale - interactive showing the sizes of things, from very tiny to huge - from NSF
If you have the chance to see one through a small telescope, it will probably look just like a fuzzy smudge to you, a piece of lint. But it is really formed of many billions of stars orbitting the center of the galaxy just as the Sun is orbiting the center of our galaxy. All the light of the galaxy comes from the stars. Elliptical galaxies are old. They formed all their stars a long time ago, and are no longer making new stars.
Galaxies like to live together in groups called clusters. In
clusters, elliptical galaxies are the most common type of galaxy. In
our group of galaxies, for example, there are no giant ellipticals,
but many dwarf ellipticals orbiting both the Milky Way and the Andromeda
galaxy.
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A Matter of Scale - interactive showing the sizes of things, from very tiny to huge - from NSF
Each elliptical galaxy is assigned a number ranging from 0 to 7 which represents how elliptical it is. The most elliptical galaxies are a 7, while a galaxy which appears circular is a 0. Their shape may tell us something about how the galaxies formed and evolved. Elliptical galaxies also come in a range of sizes from giants, which are very massive and bright, to dwarfs, which are small but which may be very numerous. In fact, ellipticals are both the largest and smallest galaxies known! We think of ellipticals as old because they have not formed any new stars recently, unlike spiral galaxies which are forming new stars even now. They appear not to have very much cool gas or dust from which to form stars.
Elliptical galaxies are the dominant type of galaxy in most clusters
and groups of galaxies. In our own Local Group, for example, there
are no large ellipticals, but many dwarf ellipticals orbiting both the
Milky Way and the Andromeda galaxy.
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A Matter of Scale - interactive showing the sizes of things, from very tiny to huge - from NSF
Last modified prior to September, 2000 by the Windows Team
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